Shell-Model Parameters of a Star with the R Coronae Borealis Type Variability

Details Shell-Model Parameters of a Star with the R Coronae Borealis Type Variability Shell-Model Parameters of a Star with the R Coronae Borealis Type Variability

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..391...39r&link_type=abstract

Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, at Eberhard

Astronomy and Astrophysics

Astronomy

Scientific paper

Based on current observational data, a revised model of spherical homogenous circumstellar shell is offered for an interpretation of visual light minima of stars with the R Coronae Borealis type variability. In this model, a light minimum is connected with the formation of one more shell in addition to the permanent one. The structure of circumstellar environment of a star with the R Coronae Borealis type variability during a visual light minimum and in a quiet state is described. Some principal physical and geometrical parameters of circumstellar shells are presented.

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