Previous Article
Convection in Stellar Evolution Models
The treatment of convection in stellar evolution calculations is briefly discussed, with emphasis on the modelling of low- and intermediate-mass stars. The specific cases of core convection during the...
Next Article
Surface Convection
What are supergranules? Why do they stand out? Preliminary results from realistic simulations of solar convection on supergranule scales (96 Mm wide by 20 Mm deep) are presented. The solar surface vel...

Convection: A Seismological Perspective

AIP Conf. Proc. -- November 9, 2007 -- Volume 948, pp. 99-110
UNSOLVED PROBLEMS IN STELLAR PHYSICS: A Conference in Honor of Douglas Gough; doi:10.1063/1.2819017

Issue Date: 9 November 2007

You are not logged in. Log in

M. H. Montgomery
Department of Astronomy, University of Texas, Austin, TX, 78712, USA
I present an overview of the close relationship which convection and stellar pulsation share. This includes the driving, damping, and modulation of oscillations in stars such as the Sun, other solar-type stars, the “classical” pulsators (e.g., Cepheids, RR Lyrae), as well as more recent results from the realm of pulsating white dwarf stars. ©2007 American Institute of Physics
BUY THIS ARTICLE   (US$28)
Download PDF (1120 kB) View Cart

KEYWORDS and PACS

Keywords
PACS
  • 97.10.Sj
    Stellar pulsations, oscillations, and stellar seismology
  • 95.30.Tg
    Thermodynamic processes, conduction, convection, equations of state in astrophysics
  • 97.20.Rp
    Faint blue stars (including blue stragglers), white dwarfs, degenerate stars, nuclei of planetary nebulae
  • YEAR: 2007

PUBLICATION DATA

ISSN:
0094-243X (print)  
Publisher:
AIP is a member of CrossRef AIP

There are no references.

CITING ARTICLES

For access to citing articles, you need to log in.
For access to citing articles, you need to Log in.