A new oscillating model suggestion for FG Vir

Details A new oscillating model suggestion for FG Vir A new oscillating model suggestion for FG Vir

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.295..473k&link_type=abstract

Astrophysics and Space Science, Volume 295, Issue 4, pp.473-484

Astronomy and Astrophysics

Astrophysics

1

Stars, Oscillations: Stars, Variables, Δ Scuti: Stars, Individual, Fg Vir, &Delta, Scuti: Stars

Scientific paper

Evolutionary stellar models of FG Vir have been developed theoretically and are compared with earlier observational results. Using the models, we performed calculations to obtain radial and non-radial adiabatic oscillation frequencies. The results show that, if the observational splitting was considered and the observational mode identifications were followed, 1.85M &sun; star models with the rotational velocities in the range from 32 to 66 kms-1 seem to be representative models of FG Vir.

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