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searching for Instability strip 19 found (298 total)

alternate case: instability strip

S Doradus (3,158 words) [view diff] case mismatch in snippet view article find links to article

lie along a diagonal band in the H–R diagram called the S Doradus Instability Strip, with the more luminous examples having hotter temperatures. The standard
GP Andromedae (546 words) [view diff] exact match in snippet view article find links to article
sequence Population I star of spectral type A3, placing it in the instability strip of the Hertzsprung-Russell diagram where Delta Scuti variables lay
HD 182475 (315 words) [view diff] exact match in snippet view article find links to article
mission: Incidence and characterisation of pulsation in the lower instability strip". Astronomy & Astrophysics. 406: 203–211. arXiv:astro-ph/0304422.
HD 224801 (726 words) [view diff] exact match in snippet view article find links to article
Andromedae; however, with a temperature of 11,000 K, it lies outside the instability strip of the HR diagram where rapidly oscillating Ap stars are located.
AE Andromedae (1,083 words) [view diff] exact match in snippet view article find links to article
to be around 20,000K, consistent with a position on the S Doradus instability strip. The star's stellar winds are strong, at 3×10−5 M☉/yr, but slow, and
HR 1884 (516 words) [view diff] case mismatch in snippet view article find links to article
Precision Velocity Study of Photometrically Stable Stars in the Cepheid Instability Strip". Astrophysical Journal. 494 (1): 342–365. Bibcode:1998ApJ...494.
BD+40°4210 (450 words) [view diff] exact match in snippet view article find links to article
appears to be extremely high, placing it on or near the S Doradus instability strip occupied by quiescent luminous blue variables. Its brightness varies
WHL0137-LS (1,294 words) [view diff] exact match in snippet view article find links to article
Upper portion of H-R Diagram showing the location of the S Doradus instability strip and the location of LBV outbursts. Main sequence is the thin sloping
Eta Orionis (730 words) [view diff] exact match in snippet view article find links to article
unusual variable spectral lines and lies with the β Cephei variable instability strip. However, it is now thought that the variable component is either
LN Andromedae (1,096 words) [view diff] exact match in snippet view article find links to article
Hertzsprung–Russell diagram at the main sequence (low luminosity) end of the same instability strip as the β Cephei stars would make high-overtone radial pulsations the
GD 66 (492 words) [view diff] case mismatch in snippet view article find links to article
S2CID 16241754. Bergeron, P.; et al. (2004). "On the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical
EC 20058-5234 (521 words) [view diff] case mismatch in snippet view article find links to article
Brassard, P. (May 1999). "Spectroscopic Studies of DB White Dwarfs: The Instability Strip of the Pulsating DB (V777 Herculis) Stars". The Astrophysical Journal
IRAS 08544−4431 (1,081 words) [view diff] exact match in snippet view article find links to article
Szabó, Gy. M.; Bedding, T. R.; Szabados, L. (2007). "Defining the instability strip of pulsating post-AGB binary stars from ASAS and NSVS photometry"
Rho Pavonis (665 words) [view diff] exact match in snippet view article find links to article
Zimmermann, M. (1995). "A catalogue of variable stars in the lower instability strip". Astronomy and Astrophysics Supplement. 109: 201. Bibcode:1995A&AS
AI Velorum (1,223 words) [view diff] exact match in snippet view article find links to article
(March 1972), "Pulsation of models in the lower part of the cepheid instability strip and properties of AI Velorum and delta Scuti stars", Astronomy and
HR 4049 (1,066 words) [view diff] exact match in snippet view article find links to article
Szabó, Gy. M.; Bedding, T. R.; Szabados, L. (2007). "Defining the instability strip of pulsating post-AGB binary stars from ASAS and NSVS photometry"
HD 5980 (3,373 words) [view diff] case mismatch in snippet view article find links to article
Diagram showing the location of HD 5980A in relation to the S Doradus Instability Strip and a number of more conventional LBVs. The likely location of HD
Eta Carinae (14,800 words) [view diff] exact match in snippet view article find links to article
luminosity. LBVs in the quiescent state lie on a narrow S Doradus instability strip, with more luminous stars being hotter. In outburst all LBVs have
Boötes (8,385 words) [view diff] exact match in snippet view article find links to article
whose members can be found both inside and outside the Delta Scuti instability strip. Lambda Boötis stars are dwarf stars that can be either spectral class