| Autor: |
Sánchez Arias, J. P., Guha, S., Kraus, M. |
| Předmět: |
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| Zdroj: |
Proceedings of the International Astronomical Union; May2024, Vol. 18 Issue S361, p251-252, 2p |
| Abstrakt: |
During the evolution of massive stars, their properties change significantly. But stellar parameters of massive stars have the biggest uncertainties in stellar astrophysics, specifically in the post-main sequence stages where blue supergiant stars are located. These stars experience mass loss events during their evolution which are supposed to be related to strange-modes instabilities. In this work, we explore the stability of oscillation modes in massive stars for different masses, and a range of mass-loss rates, with the aim to provide clues about the connection between strange modes instabilities and mass-loss events. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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