Shell structure of Be stars

Details Shell structure of Be stars Shell structure of Be stars

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pazh....1...36g&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 1, Mar. 1975, p. 36-38. In Russian.

Astronomy and Astrophysics

Astronomy

1

B Stars, Stellar Envelopes, Astronomical Models, Condensation, Electron Density (Concentration), Optical Thickness, Stellar Luminosity

Scientific paper

It is shown that the shells of Be stars should be considered as consisting of separate condensations in order to obtain better agreement between theoretical estimates of the luminosity of such stars and observations of their shells. Analytical estimates are given for some shell parameters, including the relation between electron concentration and distance from the center of a star, the optical thickness of a shell, and the number of condensations. As an example, the parameters of the shell of gamma Cas are estimated.

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