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searching for Stellar evolution 159 found (559 total)

NGC 7008 (208 words) [view diff] exact match in snippet view article find links to article

amateur and professional astronomers studying the late stages of stellar evolution and the formation of planetary nebulae. "SIMBAD Astronomical Database"

Triple-alpha process (2,689 words) [view diff] exact match in snippet view article find links to article

strong temperature dependence has consequences for the late stage of stellar evolution, the red-giant stage. For lower mass stars on the red-giant branch

Stephen Smartt (293 words) [view diff] exact match in snippet view article find links to article

1968) is an astrophysicist from Northern Ireland who specialises in stellar evolution, supernovae and time domain sky surveys. He is credited with the discovery

Sun Kwok (653 words) [view diff] exact match in snippet view article find links to article

known for his work on physics and chemistry of the late stages of stellar evolution. In 1978, he proposed a new theory on the origin of planetary nebulae

Beehive Cluster (1,932 words) [view diff] exact match in snippet view article find links to article

contain red giants and white dwarfs, which represent later stages of stellar evolution, along with many main sequence stars. Distance to M44 is often cited

The INT Photometric H-Alpha Survey (500 words) [view diff] exact match in snippet view article find links to article

provide a significant leap in our knowledge of the extreme phases of stellar evolution. The goals of the survey include: Identification of rare objects that

Circumstellar disc (3,600 words) [view diff] exact match in snippet view article find links to article

dwarfs, they indicate that planetary material survived the whole of stellar evolution. Such a disc can manifest itself in various ways. According to the

BX Circini (731 words) [view diff] exact match in snippet view article find links to article

class of star is rare, possibly because this is a brief stage of stellar evolution. Its mass has been calculated to be around 40 percent that of the

Where in the Universe Is Carmen Sandiego? (2,996 words) [view diff] exact match in snippet view article find links to article

introduced various astronomical concepts, including stars, star clusters, stellar evolution, black holes, and the Milky Way Galaxy. Both productions featured

Carbonate–silicate cycle (2,593 words) [view diff] exact match in snippet view article find links to article

worked in tandem with solar forcing, whether due to orbital changes or stellar evolution, to determine the global surface temperature. Additionally, the carbonate-silicate

Model photosphere (1,349 words) [view diff] exact match in snippet view article find links to article

and tools for studying other astrophysical problems. As a result of stellar evolution, changes in the internal structure of stars manifest themselves in

NGC 7686 (203 words) [view diff] exact match in snippet view article find links to article

Johnson, H. L.; et al. (1961), "Galactic clusters as indicators of stellar evolution and galactic structure", Bulletin of the Lowell Observatory, 5 (8):

Habitable zone (13,878 words) [view diff] exact match in snippet view article find links to article

of stellar systems may exist during the pre-main-sequence phase of stellar evolution, especially around M-dwarfs, potentially lasting for billion-year

Gennady S. Bisnovatyi-Kogan (126 words) [view diff] exact match in snippet view article find links to article

1964-1967. Bisnovatyi-Kogan's PhD thesis was titled "Late stages of stellar evolution" (1968, Keldysh Institute of Applied Mathematics). His doctoral thesis

Annapurni Subramaniam (859 words) [view diff] exact match in snippet view article find links to article

astronomer to head the institute. She works on areas like star clusters, stellar evolution and population in galaxies and Magellanic clouds. Subramaniam finished

Michael C. F. Wiescher (2,019 words) [view diff] exact match in snippet view article find links to article

nuclear physics connected with various astrophysical phenomena such as stellar evolution and explosion environments. Wiescher completed in 1969 his Abitur

Selma de Mink (467 words) [view diff] exact match in snippet view article find links to article

causing scientists to reassess the importance of binary stars in stellar evolution, De Mink has been featured in a number of popular science outlets

Convective overshoot (528 words) [view diff] exact match in snippet view article find links to article

does not fit all: Evidence for a range of mixing efficiencies in stellar evolution calculations". Astronomy & Astrophysics. 655: A29. arXiv:2107.09075

Stellar pulsation (3,258 words) [view diff] exact match in snippet view article find links to article

stars into which they gradually morph as their periods get longer. Stellar evolution and pulsation theories suggest that these irregular stars have a much

Heidelberg Institute for Theoretical Studies (1,394 words) [view diff] case mismatch in snippet view article find links to article

and to make it easily accessible to scientists. Stellar Evolution Theory (SET) The Stellar Evolution Theory group investigates the turbulent and explosive

Supernova nucleosynthesis (4,797 words) [view diff] case mismatch in snippet view article find links to article

[1968]. "Chapter 6. Calculation of Stellar Structure". Principles of Stellar Evolution and Nucleosynthesis. University of Chicago Press. ISBN 9780226109534

NGC 7142 (691 words) [view diff] exact match in snippet view article find links to article

(link) Johnson, H. L. (1961). "Galactic clusters as indicators of stellar evolution and galactic structure". Bulletin / Lowell Observatory. 5 (113): 133

WR 22 (1,401 words) [view diff] exact match in snippet view article find links to article

star systems measured in this way rather than by assumptions about stellar evolution. Despite this, the dynamical masses derived from orbital fitting vary

Bill Paxton (computer scientist) (289 words) [view diff] exact match in snippet view article

physics of stellar evolution. He is responsible for the EZ stellar evolution program and the creation of the open-source stellar evolution software Modules

Emily Levesque (1,040 words) [view diff] case mismatch in snippet view article find links to article

researching Thorne–Żytkow objects. Levesque's book Understanding Stellar Evolution, co-written with Henny Lamers and based on a series of graduate lectures

Hubert Reeves (773 words) [view diff] exact match in snippet view article find links to article

Their Relations with Stellar Evolution. London: Gordon and Breach. pp. 88pp. ISBN 0-677-02960-8. Reeves, Hubert (1968). Stellar evolution and nucleosynthesis

HH 46/47 (1,711 words) [view diff] case mismatch in snippet view article find links to article

Formation and Early Stellar Evolution. NATO Advanced Study Institute on the Physics of Star Formation and Early Stellar Evolution. Dordrecht, Netherlands:

George M. Fuller (1,132 words) [view diff] exact match in snippet view article find links to article

(Caltech). His PhD thesis entitled Nuclear weak interaction rates during stellar evolution and collapse was supervised by William A. Fowler. Fuller was from

Kappa–mechanism (529 words) [view diff] exact match in snippet view article find links to article

ISBN 978-3-540-76948-4. de Boer, Klaas Sjoerds; Seggewiss, Wilhelm (2008). Stars and stellar evolution. L'Editeur: EDP Sciences. p. 172. ISBN 978-2-7598-0356-9. LeBlanc

AE Andromedae (1,083 words) [view diff] case mismatch in snippet view article find links to article

Bomans, D. J. (2006). "LBVs in M33: Their Environments and Ages". Stellar Evolution at Low Metallicity: Mass Loss. 353: 245. Bibcode:2006ASPC..353..245B

AF Andromedae (974 words) [view diff] case mismatch in snippet view article find links to article

Bomans, D. J. (2006). "LBVs in M33: Their Environments and Ages". Stellar Evolution at Low Metallicity: Mass Loss. 353: 245. Bibcode:2006ASPC..353..245B

Nuclear astrophysics (2,254 words) [view diff] exact match in snippet view article find links to article

illustrated in the Hertzsprung-Russell diagram that classifies stages of stellar evolution. The Sun's lifetime of H burning via pp-chains is about 9 billion

NGC 2539 (758 words) [view diff] exact match in snippet view article find links to article

Mayor, M. (July 1989). "Red giants in open clusters. I. Binarity and stellar evolution in five Hyades-generation clusters : NGC 2447, 2539, 2632, 6633 and

Margaret Burbidge (2,355 words) [view diff] exact match in snippet view article find links to article

paper demonstrated that most heavier chemical elements were formed in stellar evolution. The theory they developed remains the fundamental basis for stellar

S Doradus (3,188 words) [view diff] case mismatch in snippet view article find links to article

(1975). "S Dor-type variables in other galaxies". Variable Stars and Stellar Evolution. Proceedings of the International Astronomical Union Symposia. Vol

Photodisintegration (784 words) [view diff] case mismatch in snippet view article find links to article

supernova Silicon-burning process Clayton, D. D. (1984). Principles of Stellar Evolution and Nucleosynthesis. University of Chicago Press. pp. 519. ISBN 978-0-22-610953-4

Henry Draper Medal (1,234 words) [view diff] exact match in snippet view article find links to article

his remarkably valuable contributions to knowledge of the order of stellar evolution" 1924 Arthur Stanley Eddington "For his contribution to knowledge

IC 4651 (640 words) [view diff] exact match in snippet view article find links to article

S.; Andersen, J.; Nordström, B. (April 2002). "Critical tests of stellar evolution in open clusters. III. Stellar population and dynamical evolution

Hale Telescope (2,954 words) [view diff] exact match in snippet view article find links to article

years, the Hale Telescope made many significant contributions to stellar evolution, cosmology, and high-energy astrophysics. Similarly, the telescope

Tip of the red-giant branch (645 words) [view diff] exact match in snippet view article find links to article

doi:10.1051/0004-6361/201732455. S2CID 67754889. Harpaz, Amos (1994). Stellar evolution. Peters Series. A K Peters, Ltd. pp. 103–110. ISBN 978-1-56881-012-6

Pollux b (796 words) [view diff] case mismatch in snippet view article find links to article

the International Astronomical Union. Magnetic Fields throughout Stellar Evolution. Vol. 302. pp. 359–362. arXiv:1310.6907. Bibcode:2014IAUS..302..359A

Roger Tayler (395 words) [view diff] exact match in snippet view article find links to article

versatile career in Astronomy started with pioneering studies in stellar evolution, including his discovery of semi-convection. At Harwell, his work

NGC 2360 (531 words) [view diff] case mismatch in snippet view article find links to article

Michel (1990). "Red Giants in Open Clusters. III – Binarity and Stellar Evolution in Five Intermediate-age Clusters: NGC 2360, 2423, 5822, 6811, and

Var 83 (556 words) [view diff] case mismatch in snippet view article find links to article

Bomans, D. J. (2006). "LBVs in M33: Their Environments and Ages". Stellar Evolution at Low Metallicity: Mass Loss. 353: 245. Bibcode:2006ASPC..353..245B

Red Rectangle Nebula (906 words) [view diff] exact match in snippet view article find links to article

different phases of the stellar winds (characteristic of the late stellar evolution), but its origin is still debated. On the other hand, the X-like shape

Aaron Lee Tasjan (869 words) [view diff] case mismatch in snippet view article find links to article

Karma for Cheap: Reincarnated (2019) Tasjan! Tasjan! Tasjan! (2021) ‘’Stellar Evolution’’ (2024) Luck Mansion Sessions (2017) Donelson, Marcy. "Aaron Lee

Edwin E. Salpeter (887 words) [view diff] exact match in snippet view article find links to article

February 2024. Salpeter, Edwin (1955). "The luminosity function and stellar evolution". Astrophysical Journal. 121: 161. Bibcode:1955ApJ...121..161S. doi:10

HD 149382 (586 words) [view diff] case mismatch in snippet view article find links to article

Star HD 149382—The Decisive Influence of Substellar Objects on Late Stellar Evolution". The Astrophysical Journal Letters. 702 (1): L96 – L99. arXiv:0908

Professor Aristóteles Orsini Planetarium (928 words) [view diff] exact match in snippet view article find links to article

Courses range from introductory astronomy; solar system astronomy; stellar evolution; and cosmology. There is also an exhibition room, a reading room,

Hydrogen-deficient star (1,468 words) [view diff] exact match in snippet view article find links to article

collapse. This type of hydrogen-deficient star occurs at late stages of stellar evolution. R CrB stars are hydrogen-deficient, carbon-rich stars that are notable

HR Carinae (1,509 words) [view diff] case mismatch in snippet view article find links to article

Galaxies". In Vicki E. Sherwood; Lukas Plaut (eds.). Variable Stars and Stellar Evolution. Proceedings of the International Astronomical Union Symposium No

Sjur Refsdal (389 words) [view diff] exact match in snippet view article find links to article

in 2018, with the homonymous SN Refsdal. He later started work on stellar evolution, but returned to gravitational lensing shortly before the first detection

Rudolf Kippenhahn (318 words) [view diff] exact match in snippet view article find links to article

scientific research into the computation of the structure of star and of stellar evolution. A diagram displaying how the interior of a star evolves from the

Kenneth Edgeworth (2,112 words) [view diff] case mismatch in snippet view article find links to article

of Stellar Evolution [papers I – III] (London, Monthly Notices of the Royal Astronomical Society, vol. 106, 1946) Some Aspects of Stellar Evolution [paper

Type II supernova (4,788 words) [view diff] exact match in snippet view article find links to article

observational properties is much higher than that expected from the standard stellar evolution theory. It is generally assumed that the high circumstellar density

Iodine-129 (1,670 words) [view diff] case mismatch in snippet view article find links to article

1016/j.apgeochem.2006.12.011. Clayton, Donald D. (1983). Principles of Stellar Evolution and Nucleosynthesis (2nd ed.). University of Chicago Press. pp. 75

Roche lobe (1,957 words) [view diff] exact match in snippet view article find links to article

stop mass transfer, but eventually mass transfer will start again as stellar evolution continues leading to the cases AL late overtaking The case when the

V603 Aquilae (911 words) [view diff] case mismatch in snippet view article find links to article

(1981). "Nova AQL 1918: A Nude Old Nova". Effects of Mass Loss on Stellar Evolution. Astrophysics and Space Science Library. Vol. 89. pp. 515–522. Bibcode:1981ASSL

Matter (9,519 words) [view diff] case mismatch in snippet view article find links to article

Stellar Evolution and Cosmology. Taylor & Francis. p. 202. ISBN 978-0-677-05540-4. H.S. Goldberg; M.D. Scadron (1987). Physics of Stellar Evolution and

Otto Struve (4,087 words) [view diff] exact match in snippet view article find links to article

stellar spectral class (temperature). They spurred the development of stellar evolution theory. In addition to stellar rotation, he also studied Stark effect

WR 148 (988 words) [view diff] exact match in snippet view article find links to article

stars. Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation". Astronomy and Astrophysics. 457

Yvonne Elsworth (1,100 words) [view diff] exact match in snippet view article find links to article

already contributing to a transformation in our understanding of stellar evolution. In 2011 she was awarded the Payne-Gaposchkin Medal and Prize from

ESO 3.6 m Telescope (945 words) [view diff] exact match in snippet view article find links to article

correct while the value calculated was at odds with the theory of stellar evolution. The discovery of the extrasolar planet Gliese 581 c by the team of

Age of the universe (3,880 words) [view diff] exact match in snippet view article find links to article

estimating the ages of stars. As of 2024, using the latest models for stellar evolution, the estimated age of the oldest known star is 13.8±4 billion years

W Mensae (688 words) [view diff] case mismatch in snippet view article find links to article

Southern R Coronae Borealis Variables (abstract)". Variable Stars and Stellar Evolution; Proceedings of the Symposium. 67: 147. Bibcode:1975IAUS...67..147S

Timeline of fundamental physics discoveries (2,445 words) [view diff] case mismatch in snippet view article find links to article

18842580616. Sandage, Allan (1988). "Comment on the 1925 Trumpler Paper on Stellar Evolution". Publications of the Astronomical Society of the Pacific. 100 (625):

Neon (3,862 words) [view diff] case mismatch in snippet view article find links to article

106–107. ISBN 978-0521823814. Ryan, Sean G.; Norton, Andrew J. (2010). Stellar Evolution and Nucleosynthesis. Cambridge University Press. p. 135. ISBN 978-0-521-13320-3

Chushiro Hayashi (379 words) [view diff] exact match in snippet view article find links to article

5 (2): 224–235. doi:10.1143/PTP.5.224. Hayashi, Chushiro (1961). "Stellar evolution in early phases of gravitational contraction". Publications of the

Heine's identity (326 words) [view diff] case mismatch in snippet view article find links to article

(2003). "Portent of Heine's Reciprocal Square Root Identity". 3D Stellar Evolution, ASP Conference Proceedings, held 22-26 July 2002 at University of

Raman Prinja (382 words) [view diff] exact match in snippet view article find links to article

area of research includes studies of outflows at the extremes of stellar evolution. Current projects aim to investigate the nature of mass-loss via stellar

Scientific visualization (3,071 words) [view diff] exact match in snippet view article find links to article

Hydrodynamics Calculations of Massive Star Supernovae Explosions The DJEHUTY stellar evolution code was used to calculate the explosion of SN 1987A model in three

CoRoT (14,056 words) [view diff] exact match in snippet view article find links to article

giants in this galaxy. Such theoretical populations were computed from stellar evolution models, with adopting various hypotheses to describe the successive

Degenerate matter (3,186 words) [view diff] case mismatch in snippet view article find links to article

from the original on 2012-05-11. Retrieved 2012-01-31. Lecture 17: Stellar Evolution. Discusses degenerate gases in models of stars Portals: Physics Chemistry

U Monocerotis (1,345 words) [view diff] exact match in snippet view article find links to article

521G. doi:10.1086/308451. S2CID 119408774. Bloecker, T. (1995). "Stellar evolution of low- and intermediate-mass stars. II. Post-AGB evolution". Astronomy

Static universe (1,087 words) [view diff] exact match in snippet view article find links to article

19 February 1976. ISBN 9780080873848. MacMillan, W.D. 1918. "On stellar evolution". Astrophys. J. 48: 35–49 MacMillan, W.D. 1925. "Some mathematical

Gamow factor (3,266 words) [view diff] exact match in snippet view article find links to article

ZP, 51, 204 Clayton, D. D. (Donald Delbert) (1983). Principles of stellar evolution and nucleosynthesis : with a new preface. Internet Archive. Chicago ;

Alpher–Bethe–Gamow paper (938 words) [view diff] case mismatch in snippet view article find links to article

initials of the authors' surnames, B2FH. Cameron, A. G. W. (1957). Stellar Evolution, Nuclear Astrophysics and Nucleogenesis. Chalk River Report CRL-41

Cecily Littleton (468 words) [view diff] exact match in snippet view article find links to article

structures. She also worked at Haverford College, where she studied stellar evolution. Like her great-grandfather, Littleton travelled to the Galápagos

James Croll (1,183 words) [view diff] case mismatch in snippet view article find links to article

Climate. London: Edward Stanford. 1885: Climate and Cosmology 1889: Stellar Evolution and Its Relations to Geological Time 1896: posthumous publication

Cosmic Odyssey (TV series) (1,099 words) [view diff] case mismatch in snippet view article

'extrasolar' signs of life and what such a discovery could mean. "Stellar Evolution (Lives of the Stars)" – If we could watch for millions of years, we

Merieme Chadid (773 words) [view diff] exact match in snippet view article find links to article

research aims to understand and decipher early star formation and the stellar evolution and pulsation towards of understanding of the Universe. She was listed

Donald D. Clayton (3,605 words) [view diff] case mismatch in snippet view article find links to article

elements. His pioneering textbook based on that course (Principles of Stellar Evolution and Nucleosynthesis, McGraw-Hill 1968) earned ongoing praise. In 2018

Von Zeipel theorem (351 words) [view diff] exact match in snippet view article find links to article

Bibcode:1924MNRAS..84..665V. doi:10.1093/mnras/84.9.665. Maeder, André (1999). "Stellar evolution with rotation IV: von Zeipel's theorem and anistropic losses of mass

Rome Observatory (1,530 words) [view diff] case mismatch in snippet view article find links to article

production of dust and stellar winds Models and observations of Supernovae Stellar Evolution and Astroseismology Stellar Formation and proto-stars The Sun and

Scandium (4,441 words) [view diff] case mismatch in snippet view article find links to article

22S.253V. doi:10.1002/gj.3350220619. Cameron, A.G.W. (June 1957). "Stellar Evolution, Nuclear Astrophysics, and Nucleogenesis" (PDF). CRL-41. Phoung, Sinoun;

Saul Rappaport (473 words) [view diff] case mismatch in snippet view article find links to article

astrophysics journals, are: "A New Technique for Calculations of Binary Stellar Evolution, with Application to Magnetic Braking Rappaport S, et al. Astrophysical

Katherine Freese (1,347 words) [view diff] case mismatch in snippet view article find links to article

Paolo (2008). "Stellar Structure of Dark Stars: A First Phase of Stellar Evolution Resulting from Dark Matter Annihilation". The Astrophysical Journal

Meanings of minor-planet names: 46001–47000 (419 words) [view diff] exact match in snippet view article find links to article

played by disk- and stellar-driven winds during the early phases of stellar evolution. JPL · 46920 46925 Bradyharan 1998 SS27 Brady John Haran (b. 1976)

Carina Nebula (3,723 words) [view diff] exact match in snippet view article find links to article

stars. Spectral analyses with line-blanketed model atmospheres versus stellar evolution models with and without rotation". Astronomy & Astrophysics. 457 (3):

Crafoord Prize (1,705 words) [view diff] exact match in snippet view article find links to article

pioneering contributions to the study of nuclear processes in stars and stellar evolution” — Edwin Ernest Salpeter 1998 Geosciences Don L. Anderson “for their

Joakim Edsjö (236 words) [view diff] exact match in snippet view article find links to article

implements capture, annihilation and energy transport by dark matter in a stellar evolution code. His most cited paper,"DarkSUSY: Computing Supersymmetric Dark

Mensa (constellation) (4,071 words) [view diff] exact match in snippet view article

Bibcode:1987A&A...175...60A. Higl, J.; Weiss, A. (2017). "Testing stellar evolution models with detached eclipsing binaries". Astronomy and Astrophysics

R-process (3,899 words) [view diff] case mismatch in snippet view article find links to article

doi:10.1016/0370-2693(72)90470-4. Clayton, D. D. (1968), Principles of Stellar Evolution and Nucleosynthesis, Mc-Graw-Hill, pp. 577–91, ISBN 978-0226109534

Thomas Jefferson Jackson See (1,421 words) [view diff] exact match in snippet view article find links to article

report the color of the bright star Sirius to be red as a result of stellar evolution. The Red-Sirius controversy arises because modern observations show

Hot Jupiter (5,062 words) [view diff] case mismatch in snippet view article find links to article

"Jupiter will Become a Hot Jupiter: Consequences of Post-main-sequence Stellar Evolution on Gas Giant Planets". The Astrophysical Journal. 756 (2): 132. arXiv:1207

Xenon (12,196 words) [view diff] case mismatch in snippet view article find links to article

PMID 16293758. S2CID 31226092. Clayton, Donald D. (1983). Principles of Stellar Evolution and Nucleosynthesis. University of Chicago Press. p. 604. ISBN 0-226-10953-4

R Coronae Borealis variable (2,015 words) [view diff] exact match in snippet view article find links to article

The formation of the stars themselves is also unclear. Standard stellar evolution models do not produce large luminous stars with essentially zero hydrogen

Struve–Sahade effect (520 words) [view diff] exact match in snippet view article find links to article

Bibcode:1937ApJ....85...41S. doi:10.1086/143797. Struve, Otto (1950). Stellar evolution, an exploration from the observatory. Princeton University Press.

Ursa Minor (5,858 words) [view diff] exact match in snippet view article find links to article

hydrogen and helium—its composition unexplainable by current models of stellar evolution. WD 1337+705 is a cooler white dwarf that has magnesium and silicon

Meanings of minor-planet names: 73001–74000 (419 words) [view diff] exact match in snippet view article find links to article

Roberto Buonanno (born 1947), an Italian astronomer who is an expert in stellar evolution and the director of the Rome Observatory. He created the Planetary

Evolution as fact and theory (5,249 words) [view diff] exact match in snippet view article find links to article

word evolution in a broad sense refers to processes of change, from stellar evolution to changes in language. In biology, the meaning is more specific:

Canis Major (6,870 words) [view diff] case mismatch in snippet view article find links to article

Michel (1990). "Red Giants in Open Clusters. III - Binarity and Stellar Evolution in Five Intermediate-age Clusters: NGC 2360, 2423, 5822, 6811, and

Technetium (7,651 words) [view diff] exact match in snippet view article find links to article

Schwochau 2000, pp. 286, 328. Clayton, D.D. (1983). Principles of stellar evolution and nucleosynthesis: with a new preface. University of Chicago Press

Sulfur (10,929 words) [view diff] case mismatch in snippet view article find links to article

(PDF). Yale Environmental Health & Safety. Cameron, A. G. W. (1957). "Stellar Evolution, Nuclear Astrophysics, and Nucleogenesis" (PDF). CRL-41. Mason, B

Rebecca Elson (1,150 words) [view diff] exact match in snippet view article find links to article

harvard.edu. Retrieved 23 May 2021. Henry Gee "A critical moment in stellar evolution" 2 July 1998, www.nature.com/news, on work by Elson on recently formed

Coronal mass ejection (6,828 words) [view diff] exact match in snippet view article find links to article

"Dynamics of flares on late-type dMe stars: I. Flare mass ejections and stellar evolution". Astronomy & Astrophysics. 238 (1–2): 249–255. Bibcode:1990A&A..

Metal (11,249 words) [view diff] exact match in snippet view article find links to article

as thorium and uranium. Metals condense in planets as a result of stellar evolution and destruction processes. Stars lose much of their mass when it is

Temperature (13,010 words) [view diff] case mismatch in snippet view article find links to article

a Type II supernova. Citation: Holland, Arthur; Williams, Mark. "Stellar Evolution: The Life and Death of Our Luminous Neighbors". GS265. University

Radioactive decay (9,847 words) [view diff] case mismatch in snippet view article find links to article

doi:10.1088/1674-1137/abddae. Clayton, Donald D. (1983). Principles of Stellar Evolution and Nucleosynthesis (2nd ed.). University of Chicago Press. p. 75

William Duncan MacMillan (1,545 words) [view diff] case mismatch in snippet view article find links to article

1090/S0002-9947-1918-1501098-4. MacMillan, William Duncan (1918). "On Stellar Evolution". Astrophysical Journal. 48: 35. Bibcode:1918ApJ....48...35M. doi:10

Universe (15,970 words) [view diff] case mismatch in snippet view article find links to article

ISBN 978-0-521-57883-7. Clayton, Donald D. (1983). Principles of Stellar Evolution and Nucleosynthesis. The University of Chicago Press. pp. 362–435

Arthur Eddington (6,598 words) [view diff] exact match in snippet view article find links to article

powerful tool for further investigation, particularly in issues of stellar evolution. The confirmation of his estimated stellar diameters by Michelson

Gaia (spacecraft) (8,151 words) [view diff] exact match in snippet view article

samples. To permit a better understanding of the more rapid stages of stellar evolution (such as the classification, frequency, correlations and directly

Enrique García-Berro (969 words) [view diff] exact match in snippet view article find links to article

and made a number of important contributions to the knowledge of stellar evolution, with a particular emphasis on white dwarfs. During a stay at the

Uranium (12,428 words) [view diff] case mismatch in snippet view article find links to article

1103/RevModPhys.29.547. Clayton, Donald D. (1968). Principles of Stellar Evolution and Nucleosynthesis. New York: Mc-Graw-Hill. pp. 577–91. ISBN 978-0226109534

Decay chain (3,963 words) [view diff] exact match in snippet view article find links to article

with the birth of the first stars. The nuclear furnaces that power stellar evolution were necessary to create large quantities of all elements heavier

String theory (15,263 words) [view diff] exact match in snippet view article find links to article

particle or radiation can escape. In the currently accepted models of stellar evolution, black holes are thought to arise when massive stars undergo gravitational

Cosmic age problem (2,382 words) [view diff] exact match in snippet view article find links to article

However, in the 1960s and onwards, new developments in the theory of stellar evolution enabled age estimates for large star clusters called globular clusters:

Helioseismology (5,445 words) [view diff] case mismatch in snippet view article find links to article

"The Solar Chemical Composition", Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis, 336: 25, Bibcode:2005ASPC..336...25A Asplund

Renewable energy (16,351 words) [view diff] exact match in snippet view article find links to article

energy for the remaining lifespan of the sun on the main sequence of stellar evolution. Artificial photosynthesis uses techniques including nanotechnology

Chandrasekhar family (1,063 words) [view diff] exact match in snippet view article find links to article

structure and evolution of the stars". His mathematical treatment of stellar evolution yielded many of the best current theoretical models of the later evolutionary

Ian Glass (1,394 words) [view diff] exact match in snippet view article find links to article

period-luminosity relationship for Mira-like variables in the LMC. Late stages of stellar evolution, Calgary, Canada, 2–5 June 1986. Dordrecht, Netherlands: D. Reidel

Beta decay transition (2,080 words) [view diff] exact match in snippet view article find links to article

}}&{\text{Gamow–Teller Decay}}\end{cases}}} Clayton, Donald D. (1983). Principles of stellar evolution and nucleosynthesis : with a new preface (University of Chicago Press ed

Breeder reactor (8,330 words) [view diff] exact match in snippet view article find links to article

energy for the remaining lifespan of the sun on the main sequence of stellar evolution. In broad terms, spent nuclear fuel has three main components. The

Initial mass function (3,568 words) [view diff] exact match in snippet view article find links to article

S2CID 15276163. Salpeter, Edwin (1955). "The luminosity function and stellar evolution". Astrophysical Journal. 121: 161. Bibcode:1955ApJ...121..161S. doi:10

Thorium (16,481 words) [view diff] case mismatch in snippet view article find links to article

doi:10.1103/RevModPhys.29.547. Clayton, D. D. (1968). Principles of Stellar Evolution and Nucleosynthesis. McGraw-Hill Education. pp. 577–591. ISBN 978-0-226-10953-4

Nuclear binding energy (7,077 words) [view diff] exact match in snippet view article find links to article

abundant; they (and other nuclei heavier than helium) have formed in stellar evolution events like supernova explosions preceding the formation of the Solar

Shamakhy Astrophysical Observatory (2,432 words) [view diff] exact match in snippet view article find links to article

conclusions were drawn about the physical nature of the end product of stellar evolution. It is shown that during the collapse, during the formation of a neutron

Heavy metals (12,567 words) [view diff] exact match in snippet view article find links to article

thorium and uranium. Heavy metals condense in planets as a result of stellar evolution and destruction processes. Stars lose much of their mass when it is

X-ray astronomy (8,115 words) [view diff] exact match in snippet view article find links to article

formed stars are known as pre-main-sequence stars during the stage of stellar evolution before they reach the main-sequence. Stars in this stage (ages <10

History of astronomy (10,388 words) [view diff] exact match in snippet view article find links to article

Successful models were developed to explain the interiors of stars and stellar evolution. Cecilia Payne-Gaposchkin first proposed that stars were made primarily

Abiogenesis (21,778 words) [view diff] exact match in snippet view article find links to article

enough regions on the early Earth that large ice cover could be found. Stellar evolution models predict that the Sun's luminosity was ~25% weaker than it is

List of galaxies (6,315 words) [view diff] case mismatch in snippet view article find links to article

(1999). "The First 50 Years at Palomar: 1949–1999 the Early Years of Stellar Evolution, Cosmology, and High-Energy Astrophysics". Annual Review of Astronomy

Kardashev scale (16,908 words) [view diff] exact match in snippet view article find links to article

original on 2015-09-24. Retrieved 2023-08-27. Zuckerman, B. (1985). "Stellar evolution – Motivation for mass interstellar migrations". Quarterly Journal

Mario Runco Jr. (3,311 words) [view diff] exact match in snippet view article find links to article

X-Ray Spectrometer (DXS). This astronomical instrument for studying stellar evolution scanned the local vicinity of our Milky Way galaxy and recorded the

Angela Speck (1,275 words) [view diff] case mismatch in snippet view article find links to article

Components in the PPN/PN Dust Shells", Post-AGB Objects as a Phase of Stellar Evolution, vol. 265, Springer Netherlands, pp. 339–342, arXiv:astro-ph/0010208

Manuel Foster Observatory (3,654 words) [view diff] case mismatch in snippet view article find links to article

Observations of the Nebulae and Their Bearing upon the Problem of Stellar Evolution", Popular Astronomy, 23: 553–562, Bibcode:1915PA.....23..553W. Campbell

Harm Habing (320 words) [view diff] exact match in snippet view article find links to article

Leiden Observatory, his interests included masers, late stages of stellar evolution (such as OH/IR stars), and star formation. Habing was principal investigator

Andrea Kritcher (1,141 words) [view diff] case mismatch in snippet view article find links to article

(2020-08-16). "1.1 Million Joules of UV Laser Energy: Shedding Light on Stellar Evolution and "Cosmic Clocks"". SciTechDaily. Retrieved 2022-12-10. Behr, Peter

Scott Jay Kenyon (1,911 words) [view diff] exact match in snippet view article find links to article

090189.002031. Reipurth, B. (1990), "FU Orionis eruptions and early stellar evolution", Flare Stars in Star Clusters, 137: 229, Bibcode:1990IAUS..137..229R

List of exoplanet extremes (7,881 words) [view diff] case mismatch in snippet view article find links to article

the International Astronomical Union. Magnetic Fields throughout Stellar Evolution. Vol. 302. pp. 359–362. arXiv:1310.6907. Bibcode:2014IAUS..302..359A

History of Solar System formation and evolution hypotheses (7,872 words) [view diff] exact match in snippet view article find links to article

fuel, so planetary nebulae came to be understood as a final stage of stellar evolution. Spectroscopic observations show that all planetary nebulae are expanding

Amanda Bauer (2,392 words) [view diff] exact match in snippet view article find links to article

found that a galaxy's position within the galactic cluster affected stellar evolution within that galaxy: the closer a galaxy is to the center of a cluster

List of alumni of Trinity College, Cambridge (3,747 words) [view diff] exact match in snippet view article find links to article

in Oxford Sir James Jeans (1877–1946), astronomer, mathematician; stellar evolution John Edensor Littlewood (1885–1977), mathematician; Fourier Series

Cosmological lithium problem (2,736 words) [view diff] case mismatch in snippet view article find links to article

(2005-01-20). "Implications of WMAP Observations on Li Abundance and Stellar Evolution Models". The Astrophysical Journal. 619 (1): 538–548. arXiv:astro-ph/0409672

Pea galaxy (13,064 words) [view diff] exact match in snippet view article find links to article

N. Grevesse; A.J. Sauval (2005). "Cosmic abundances as records of stellar evolution and nucleosynthesis". ASP Conference Series. 336: 25. arXiv:astro-ph/0410214

Meanings of minor-planet names: 8001–9000 (435 words) [view diff] exact match in snippet view article find links to article

stellar spectroscopy, stellar atmospheres and observable effects of stellar evolution. Her later interests were the ultraviolet and optical spectroscopy

Malmquist bias (4,129 words) [view diff] exact match in snippet view article find links to article

Bibcode:1925MeLuF.106....1M. Salpeter, Edwin (1955). "The luminosity function and stellar evolution". The Astrophysical Journal. 121: 161. Bibcode:1955ApJ...121..161S

Index of branches of science (8,636 words) [view diff] exact match in snippet view article find links to article

forces in nonmoving systems Stellar astronomy – Study of stars and stellar evolution Stemmatics, also known as Stemmatology – Identification of textual

LZ Cephei (534 words) [view diff] exact match in snippet view article find links to article

evolved massive binary LZ Cephei. Testing the effects of binarity on stellar evolution". Astronomy & Astrophysics. 533. arXiv:1106.6162. Bibcode:2011A&A

Charles Robert O'Dell (1,150 words) [view diff] exact match in snippet view article find links to article

planets). He used observations and theory to establish their role in stellar evolution. Much of his current activity is focused on the nearby star-formation

Immo Appenzeller (877 words) [view diff] exact match in snippet view article find links to article

contributions to several research fields, including star formation, stellar evolution, high redshift galaxies, active galaxies and quasars, massive luminous

Non-planetary abiogenesis (1,315 words) [view diff] exact match in snippet view article find links to article

life" could be observed deviations from predictions of models of stellar evolution, such as anomalies in luminosity. Authors themselves characterize

A. B. R. Hazarika (871 words) [view diff] exact match in snippet view article find links to article

and evolution of the neutron stars. His mathematical treatment of stellar evolution yielded many of the current theoretical models of the later evolutionary

Superflare (7,656 words) [view diff] exact match in snippet view article find links to article

temperature and surface gravity change over the lifetime of a star, stellar evolution theory allows an estimate of the age of a star: in most cases the

UGC 9684 (1,506 words) [view diff] case mismatch in snippet view article find links to article

Population Synthesis Modeling. I. The Relevance of Uncertain Aspects of Stellar Evolution and the Initial Mass Function to the Derived Physical Properties of

Washington Conference on Theoretical Physics (1,505 words) [view diff] case mismatch in snippet view article find links to article

Geophysics and the Interior of the Earth 1941 Elementary Particles 1942 Stellar Evolution and Cosmology Gap due to World War II 1946 Physics on Living Matter

MWC 560 (1,457 words) [view diff] case mismatch in snippet view article find links to article

"Possible Pulsations of the M Giant in MWC 560", Symbiotic Stars Probing Stellar Evolution, ASP Conference Proceedings, Vol. 303. Held 27-31 May 2002 at Isaac

List of minor planets: 549001–550000 (662 words) [view diff] exact match in snippet view article find links to article

astronomer at the Konkoly Observatory. The main areas of his research were stellar evolution and the observation of variable stars. IAU · 549185 549228 Labuda