Skip to content Skip to navigation
University of Warwick
  • Study
  • |
  • Research
  • |
  • Business
  • |
  • Alumni
  • |
  • News
  • |
  • About

University of Warwick
Publications service & WRAP

Highlight your research

  • WRAP
    • Home
    • Search WRAP
    • Browse by Warwick Author
    • Browse WRAP by Year
    • Browse WRAP by Subject
    • Browse WRAP by Department
    • Browse WRAP by Funder
    • Browse Theses by Department
  • Publications Service
    • Home
    • Search Publications Service
    • Browse by Warwick Author
    • Browse Publications service by Year
    • Browse Publications service by Subject
    • Browse Publications service by Department
    • Browse Publications service by Funder
  • Statistics
  • Help & Advice
University of Warwick

The Library

  • Login

Finding the instability strip for accreting pulsating white dwarfs from Hubble Space Telescope and optical observations

Tools
- Tools
+ Tools

Szkody, Paula, Mukadam, Anjum S., Gänsicke, B. T. (Boris T.), Henden, Arne A., Templeton, Matthew, Holtzman, J. (Jon), Montgomery, Michael H., Howell, Steve B., Nitta, Atsuko, Sion, Edward M., Schwartz, Richard Dean, 1941- and Dillon, W. (William). (2010) Finding the instability strip for accreting pulsating white dwarfs from Hubble Space Telescope and optical observations. The Astrophysical Journal, Vol.710 (No.1). pp. 64-77. ISSN 0004-637X

Full text not available from this repository.
Official URL: http://dx.doi.org/10.1088/0004-637X/710/1/64

Abstract

Time-resolved low resolution Hubble Space Telescope ultraviolet spectra together with ground-based optical photometry and spectra are used to constrain the temperatures and pulsation properties of six cataclysmic variables containing pulsating white dwarfs (WDs). Combining our temperature determinations for the five pulsating WDs that are several years past outburst with past results on six other systems shows that the instability strip for accreting pulsating WDs ranges from 10,500 to 15,000 K, a wider range than evident for ZZ Ceti pulsators. Analysis of the UV/optical pulsation properties reveals some puzzling aspects. While half the systems show high pulsation amplitudes in the UV compared to their optical counterparts, others show UV/optical amplitude ratios that are less than one or no pulsations at either wavelength region.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science > Physics
Library of Congress Subject Headings (LCSH): Dwarf novae, Ultraviolet stars, White dwarf stars, Stellar oscillations
Journal or Publication Title: The Astrophysical Journal
Publisher: Institute of Physics Publishing, Inc.
ISSN: 0004-637X
Date: 10 February 2010
Volume: Vol.710
Number: No.1
Number of Pages: 14
Page Range: pp. 64-77
Identification Number: 10.1088/0004-637X/710/1/64
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access
Funder: United States. National Aeronautics and Space Administration (NASA), Association of Universities for Research in Astronomy (AURA), Particle Physics and Astronomy Research Council (Great Britain) (PPARC)
Grant number: HST-GO-11163.01 (NASA), NAS 5-26555 (NASA)
URI: http://wrap.warwick.ac.uk/id/eprint/16564

Data sourced from Thomson Reuters' Web of Knowledge

Request changes to a record

Actions (login required)

View Item View Item
twitter

Email us: publications@warwick.ac.uk
Contact Details
About Us