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Longer titles found: Metallicity distribution function (view)

searching for Metallicity 17 found (3853 total)

alternate case: metallicity

NGC 4429 (413 words) [view diff] no match in snippet view article find links to article

NGC 4429 is a lenticular galaxy located about 55 million light-years away in the constellation of Virgo. NGC 4429 is tilted at an inclination of about
NGC 4458 (645 words) [view diff] no match in snippet view article find links to article
NGC 4458 is an elliptical galaxy located about 54 million light-years away in the constellation of Virgo. It was discovered by astronomer William Herschel
NGC 4478 (506 words) [view diff] no match in snippet view article find links to article
NGC 4478 is an elliptical galaxy located about 50 million light-years away in the constellation Virgo. NGC 4478 was discovered by astronomer William Herschel
Names for sets of chemical elements (528 words) [view diff] no match in snippet view article find links to article
There are currently 118 known chemical elements with a wide range of physical and chemical properties. Amongst this diversity, scientists have found it
Hercules (dwarf galaxy) (841 words) [view diff] exact match in snippet view article
consists mainly of old stars formed more than 12 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.58 ± 0.51, which means
LAMOST 1 (136 words) [view diff] exact match in snippet view article find links to article
light years distant in the Milky Way. The stars have similar age and metallicity. The stars were discovered in spectra from the Large Sky Area Multi-Object
Palomar 14 (358 words) [view diff] exact match in snippet view article find links to article
about 3–4 billion years younger than a typical galactic cluster. The metallicity of the cluster is [Fe/H] = −1.50, indicating a lower abundance of elements
Smith's Cloud (698 words) [view diff] exact match in snippet view article find links to article
hypothesis; these measurements show that the Smith Cloud has an average metallicity of one half of the solar value, indicating that its gas originates in
Canes Venatici II (659 words) [view diff] exact match in snippet view article find links to article
consists mainly of old stars formed more than 12 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.19±0.58, which means
Y Sagittarii (469 words) [view diff] exact match in snippet view article find links to article
the Sun. The star's metal content is similar to Sun, with an index of metallicity [Fe / H] = +0.05. For other metals tested, it shows some overabundance
List of planet types (528 words) [view diff] exact match in snippet view article find links to article
deuterium (currently calculated to be 13 Jupiter masses for objects of solar metallicity) that orbit stars, brown dwarfs or stellar remnants and that have a mass
Canes Venatici I (821 words) [view diff] exact match in snippet view article find links to article
consists mainly of old stars formed more than 10 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.08 ± 0.02, which means
HAT-P-12b (548 words) [view diff] exact match in snippet view article find links to article
core mass of 11.3+2.6 −2.1 M🜨 and is moderately irradiated by its low-metallicity host star. Therefore, HAT-P-12b is most likely an H/He-dominated planet
Ursa Major II Dwarf (598 words) [view diff] exact match in snippet view article find links to article
consists mainly of old stars formed at least 10 billion years ago. The metallicity of these old stars is also very low at [Fe/H] ≈ −2.44 ± 0.06, which means
Strongly correlated material (1,105 words) [view diff] exact match in snippet view article find links to article
properties, such as metal-insulator transitions, heavy fermion behavior, half-metallicity, and spin-charge separation. The essential feature that defines these
T Coronae Borealis (1,305 words) [view diff] exact match in snippet view article find links to article
George; Harrison, Tanya; Munari, Ulisse; Vanture, Andrew (2008). "The Metallicity and Lithium Abundances of the Recurring Novae T CrB and RS Oph". Publications
IRAS 05280–6910 (587 words) [view diff] exact match in snippet view article find links to article
content, and mass-loss rates of evolved AGB and RSG stars at varying metallicity". Monthly Notices of the Royal Astronomical Society. 465 (1): 403–433