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Higher Vibrational Modes In RR Lyrae Stars

Published online by Cambridge University Press:  15 February 2018

S. A. Glasner
Affiliation:
The Racah Institute of Physics, Jerusalem, Israel
J. R. Buchler
Affiliation:
Physics Department, University of Florida, Gainesville, Florida, USA

Abstract

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A simple method for computing the full spectrum of the linear (nonadiabatic) radial modes is implemented and tested on RR Lyrae models. The growthrates of the vibrational modes display unexpected, but physically correct undulations as a function of period, with the 8th through 10th overtones almost unstable. Caution must be exercised when only a small number of meshpoints is used, or when the meshpoints are not well distributed, as some of these overtones may become unstable, clearly an artifact of the differencing. The role that such unstable high overtones can play in hydrodynamic calculations is demonstrated.

Type
Theoretical Breakthroughs
Copyright
Copyright © Cambridge University Press 1993