Previous Article
Periodic Light Variability in Twelve Carbon-rich Proto-Planetary Nebulae
We present the results of a long-term (14 year) photometric monitoring program of 12 carbon-rich proto-planetary nebulae (PPNs). PPNs are objects in the evolutionary transition between the AGB and pla...
Next Article
Seismology of White Dwarfs: The ZZ Ceti Stars
We calculate an extensive adiabatic model grid for pulsating white dwarfs with H dominated atmospheres, the ZZ Ceti stars. We developed a new approach for asteroseismology, using the relative observed...

White Dwarf and Pre-White Dwarf Pulsations

AIP Conf. Proc. -- September 16, 2009 -- Volume 1170, pp. 605-615
STELLAR PULSATION: CHALLENGES FOR THEORY AND OBSERVATION: Proceedings of the International Conference; doi:10.1063/1.3246571

Issue Date: 16 September 2009

You are not logged in. Log in

M. H. Montgomery
Department of Astronomy and McDonald Observatory, University of Texas, Austin TX 78712, USA and Delaware Asteroseismic Research Center, Mt. Cuba Observatory, Greenville, DE, USA
In this review I describe the basic properties of white dwarfs and their pulsations. I then discuss some of the areas in which the pulsations can provide meaningful results, such as internal chemical profiles, possible emission of “exotic” particles, planet detection, crystallization, convection, accretion, and cosmochronology. ©2009 American Institute of Physics
BUY THIS ARTICLE   (US$24)
Download PDF (2428 kB) View Cart

KEYWORDS and PACS

Keywords
PACS
  • 97.20.Rp
    Faint blue stars (including blue stragglers), white dwarfs, degenerate stars, nuclei of planetary nebulae
  • 95.55.Qf
    Photometric, polarimetric, and spectroscopic instrumentation for astronomy
  • 97.10.Sj
    Stellar pulsations, oscillations, and stellar seismology
  • YEAR: 2009

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.