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...

Full description

Bibliographic Details

Published in:	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
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Massive stars Pulsating variable stars
Online Access:	https://doi.org/10.3847/1538-4365/ad1f66