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
  • Help & Advice
University of Warwick

The Library

  • Login
  • Admin

HS 0943+1404 : a true intermediate polar

Tools
- Tools
+ Tools

Rodríguez-Gil, P., Gaensicke, B. T., Hagen, H.-J., Nogami, D., Torres, M. A. P., Lehto, H., Aungwerojwit, A., Littlefair, S. P., Araujo-Betancor, S. and Engels, Dieter (2005) HS 0943+1404 : a true intermediate polar. Astronomy & Astrophysics, Vol.440 (No.2). pp. 701-709. doi:10.1051/0004-6361:20053141 ISSN 0004-6361.

[img] PDF
WRAP_Rodriguez-Gil_96_HS_0943+1404.pdf - Requires a PDF viewer.

Download (1120Kb)
Official URL: http://dx.doi.org/10.1051/0004-6361:20053141

Request Changes to record.

Abstract

We have identified a new intermediate polar, HS 0943+1404, as part of our ongoing search for cataclysmic variables in the Hamburg Quasar Survey. The orbital and white dwarf spin periods determined from time-resolved photometry and
spectroscopy are P orb 250 min and P spin = 69.171 ± 0.001 min, respectively. The combination of a large ratio P spin /P orb 0.3 and a long orbital period is very unusual compared to the other known intermediate polars. The magnetic moment of the white dwarf is estimated to be µ 1 ∼
10 34 Gcm 3, which is in the typical range of polars. Our extensive photometry shows that HS 0943+1404 enters into deep (∼3 mag) low states, which are also a characteristic feature of polars. We therefore suggest that the system is a true “intermediate” polar that will eventually synchronise, that is, a transitional object between intermediate polars and polars. The optical spectrum of HS 0943+1404 also exhibits a number of unusual emission lines, most noticeably N II λ5680, which is likely to reflect enhanced nitrogen abundances in the envelope of the secondary.

Item Type: Journal Article
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Library of Congress Subject Headings (LCSH): Cataclysmic variable stars
Journal or Publication Title: Astronomy & Astrophysics
Publisher: EDP Sciences
ISSN: 0004-6361
Official Date: September 2005
Dates:
DateEvent
September 2005Published
Volume: Vol.440
Number: No.2
Page Range: pp. 701-709
DOI: 10.1051/0004-6361:20053141
Status: Peer Reviewed
Access rights to Published version: Open Access (Creative Commons)
Funder: Particle Physics and Astronomy Research Council (Great Britain) (PPARC), Deutsche Forschungsgemeinschaft (DFG), United States. National Aeronautics and Space Administration (NASA)
Grant number: Re 353/11 (DFG), Re 353/22 (DFG), NAG5-9930 (NASA)

Request changes or add full text files to a record

Repository staff actions (login required)

View Item View Item

Downloads

Downloads per month over past year

View more statistics

twitter

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