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...

書目詳細資料
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

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