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...
| Autori principali: | , , , , , |
|---|---|
| Natura: | Articolo |
| Lingua: | English |
| Pubblicazione: |
IOP Publishing
2024-01-01
|
| Serie: | The Astrophysical Journal Supplement Series |
| Soggetti: | |
| Accesso online: | https://doi.org/10.3847/1538-4365/ad1f66 |