γ Bootis: Asteroseismology with a 1-m Class Telescope

Details γ Bootis: Asteroseismology with a 1-m Class Telescope γ Bootis: Asteroseismology with a 1-m Class Telescope

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..948..455d&link_type=abstract

UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough. AIP Conference Proceedings, Volume 948, pp. 455-4

Physics

Astronomical And Space-Research Instrumentation, Pulsations, Oscillations, And Stellar Seismology, Stellar Rotation, Helioseismology, Pulsations, And Shock Waves

Scientific paper

High-resolution spectroscopic observations carried out in 2005, allowed Ventura et al. (2007) to identify oscillation modes on the rapidly rotating δ Scuti star γ Bootis. Here we consider the theoretical interpretation of the observed oscillation spectrum based on structure models and oscillation frequencies calculated by including effects due to the fast rotation.

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