TY  - CHAP 
AU  - Mirouh, Giovanni M.
AU  - Reese, Daniel R.
AU  - Rieutord, Michel
AU  - Ballot, Jérôme
PY  - 2017
UR  - https://hdl.handle.net/10481/111813
AB  - Early-type stars generally tend to be fast rotators. In these stars, mode identification is very challenging as the effects of rotation are not well known. We consider here the example of α Ophiuchi, for which dozens of oscillation frequencies have...
LA  - eng
KW  - asteroseismology
KW  - stars:rotation
KW  - Astrophysics - Solar and Stellar Astrophysics
TI  - Non-adiabatic oscillations of fast-rotating stars: the example of Rasalhague
DO  - 10.48550/arXiv.1711.06053
ER  -