The effect of convection on pulsational stability

Abstract

A review on the current state of mode physics in classical pulsators is presented. Two, currently in use, time-dependent convection models are compared and their applications on mode stability are discussed with particular emphasis on the location of the Delta Scuti instability strip.

arXiv commentAccepted for publication in CoAst (invited paper), 9 pages, 4 figures

Cited by in corpus (1)

• Exploring the convective core of the high-amplitude $\delta$ Scuti star TIC 120857354 with asteroseismology