Seismic evidence for a rapidly rotating core in a lower-giant-branch star observed with kepler
Rotation is expected to have an important influence on the structure and the evolution of stars. However, the mechanisms of angular momentum transport in stars remain theoretically uncertain and very complex to take into account in stellar models. To achi
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|Access Rights:||Open Access|
|01_Deheuvels_Seismic_evidence_for_a_rapidly_2012.pdf||1.45 MB||Adobe PDF|
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