Inference for stellar opacities from seismic studies of the hybrid β Cep/SPB pulsators
We present a comprehensive seismic study of the three pulsating stars of β Cep/SPB type: v Eridani, 12 Lacertae and γ Pegasi. Models with the modified mean opacity profile are constructed in order to account for both the observed frequency range and the values of some individual frequencies. To decr...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
EDP Sciences
2017-01-01
|
| Series: | EPJ Web of Conferences |
| Online Access: | https://doi.org/10.1051/epjconf/201715206005 |