Hostname: page-component-5cf477f64f-54txb Total loading time: 0 Render date: 2025-04-05T00:36:51.042Z Has data issue: false hasContentIssue false
  • English
  • Français

A survey of RR Lyrae models

Published online by Cambridge University Press:  15 February 2018

G. Bono  and
R.F. Stellingwerf
G. Bono
Affiliation:
Trieste Astronomical Observatory, Italy
R.F. Stellingwerf
Affiliation:
Los Alamos National Laboratory, NM

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

An extensive grid of non-linear pulsating models of RR Lyrae stars have been computed. To simulate the outer regions of these variables a non-local and time-dependent treatment of convective transport has been adopted. In this poster we briefly describe some new features of the instability strip (IS).

Type
Theoretical Breakthroughs
Information
International Astronomical Union Colloquium , Volume 139: New Perspectives on Stellar Pulsation and Pulsating Variable Stars , 1993 , pp. 262
Copyright
Copyright © Cambridge University Press 1993