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Stellar Structure and RR Lyrae Masses

Published online by Cambridge University Press:  15 February 2018

Ben Dorman
Ben Dorman*
Affiliation:
Astronomy Department, U. Virginia

Abstract

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I describe qualitatively the constraints on RR Lyrae masses that arise from consideration of the interior structure of Horizontal Branch (HB) stars. Briefly, the stellar models lying within the temperature range of the instability strip are slightly less massive than those with deep exterior convection zones. I discuss therefore what brings about the existence of these zones in the models.

Type
Theoretical Breakthroughs
Information
International Astronomical Union Colloquium , Volume 139: New Perspectives on Stellar Pulsation and Pulsating Variable Stars , 1993 , pp. 309 - 311
Copyright
Copyright © Cambridge University Press 1993

References

Buonanno, R., Corsi, C.E., and Fusi Pecci, F. 1985 A&A 145, 97 Google Scholar
Cox, A.N. 1991 ApJ, 381, L71 Google Scholar
Dorman, B. 1992a ApJS, 80, 701 Google Scholar
Dorman, B. 1992b ApJS, 81, 221 CrossRefGoogle Scholar
Kovács, G., Buchler, J.R., and Marom, A. 1991 A&A 252, L27 Google Scholar
Simon, N.R., 1992, this volumeGoogle Scholar
Stetson, P.B. 1991 in Precision Photometry: Astrophysics of the Galaxy, eds. Philip, A.G.D., Upgren, A.R. & Janes, K.A. (New York: Davis), p.69 Google Scholar