The limits of validity of the Frequency Ratio Method: The particular case of γ Doradus stars

Details The limits of validity of the Frequency Ratio Method: The particular case of γ Doradus stars The limits of validity of the Frequency Ratio Method: The particular case of γ Doradus stars

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008an....329..545s&link_type=abstract

Astronomische Nachrichten, Vol.329, Issue 5, p.545

Astronomy and Astrophysics

Astronomy

1

Stars: Evolution, Stars: Fundamental Parameters, Stars: Interiors, Stars: Oscillations, Stars: Rotation

Scientific paper

This work provides a general vision of the limits of validity of the Frequency Ratio Method applied to the g-mode pulsators in asymptotic regime, the γ Doradus stars. In particular, the work is mainly focused on the role of rotation which is found one of the most important source of uncertainty of the method. The particular case of the moderately rotating γ Doradus star HD 48501 is discussed.

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