Asteroseismology: ground based observational methods

S. Frandsen
1997 Symposium - International astronomical union  
The improvement in observational techniques to study pulsations in solarlike stars is discussed. For higher mass stars the problem is to allocate specific eigenmodes to a set of observed frequencies. Additional observables can be used to sort out the present ambiguities.
doi:10.1017/s0074180900061258 fatcat:kk4aza5uv5g5pjinvuz724yusu