Observational Properties of 155 β Cephei Pulsating Variable Stars

β Cephei pulsating variable (BCEP) stars are the most massive pulsating variable stars in the main sequence, exhibiting both p - and g -mode pulsations. In this study, we identified 155 BCEP stars or candidates using data from TESS and Gaia, of which 83 were first confirmed as BCEP stars. They have...

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發表在:	The Astrophysical Journal Supplement Series
Main Authors:	Xiang-dong Shi, Sheng-bang Qian, Li-ying Zhu, Lin-jia Li, Er-gang Zhao, Wen-xu Lin
格式:	Article
語言:	英语
出版:	IOP Publishing 2024-01-01
主題:	Massive stars Pulsating variable stars
在線閱讀:	https://doi.org/10.3847/1538-4365/ad1f66