Theoretical Models of W-Virginis Stars

Details Theoretical Models of W-Virginis Stars Theoretical Models of W-Virginis Stars

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cto..conf..246b&link_type=abstract

Cepheids: Theory and Observations, Proceedings of IAU Colloquium No. 82, held 29 May - 1 June, 1984 in Toronto, Canada. Edited

Physics

9

Scientific paper

W Virginis variables are the population II counterparts of the classical
Cepheids, although they do not show quite the same trends as are seen in
the latter. The paper summarises the results of a series of hydrodynamic
(nonlinear) models constructed in an attempt to reproduce the observed
characteristics of these stars.

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