A Possible Extension of the Stellingwerf One-Zone Stellar Model

Details A Possible Extension of the Stellingwerf One-Zone Stellar Model A Possible Extension of the Stellingwerf One-Zone Stellar Model

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..349..313p&link_type=abstract

Astrophysics of Variable Stars, Pecs, Hungary, 5-10 September 2005, Sterken, C. and Aerts, C. (eds). ASP Conference Series, Vol.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Stellingwerf one-zone stellar model is being extended by considering a slow and uniform rotation that leads to a very small oblateness of the star. The matter in the core-surrounding shell is supposed to consist of a mixture of ideal gas and radiation. This one-zone stellar pulsation model is proposed as a tool to investigate the linear stability, as well as the factors affecting thermal variation of pulsating stars. Linear and non-linear analyses of the resulting equations are described.

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