Other
Scientific paper
Jun 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005japa...26..241h&link_type=abstract
Journal of Astrophysics and Astronomy, Vol. 26, Issue 2-3, p. 2005
Other
4
Stars: Variables: Δ, Scuti, Stars: Oscillations, Variables: Other
Scientific paper
We give an overview of past and present efforts to make seismology of δ Scuti and γ Doradus stars possible. Previous work has not led to the observational detection and identification of a sufficient number of pulsation modes for these pulsators for the construction of unique seis-mic models. However, recent efforts including large ground-based obser-vational campaigns, work on pre-main sequence pulsators, asteroseismic satellite missions, theoretical advances on mode identification methods, and the discovery of a star showing simultaneous self-excited δ Scuti and γ Doradus oscillations suggest that we may be able to explore the interiors of these pulsators in the very near future.
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