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. © 2007 American Institute of Physics.
γ Bootis: Asteroseismology: with a 1-M class telescope
Catanzaro G.;
2007-01-01
Abstract
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. © 2007 American Institute of Physics.File in questo prodotto:
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