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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| Автори: | , , , , , |
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| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
IOP Publishing
2024-01-01
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| Серія: | The Astrophysical Journal Supplement Series |
| Предмети: | |
| Онлайн доступ: | https://doi.org/10.3847/1538-4365/ad1f66 |
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