Instability strip for pre-main-sequence stars

Details Instability strip for pre-main-sequence stars Instability strip for pre-main-sequence stars

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006coast.147...69g&link_type=abstract

Communications in Asteroseismology, vol. 147, p. 69-71

Computer Science

8

Scientific paper

We apply the Time Dependent Convection (TDC) treatment presented in Grigahcene et al. (2005) to the study of Pre-main sequence pulsating stars. The stabilization of the p-modes at the red edge of the Instability Strip (IS) is obtained by our models. The theoretical IS obtained with Mixing Length (ML) parameter alpha=1.8 is compared to observations and a good agreement is obtained.

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