van Spaandonk, Lieke, Steeghs, D., Marsh, T. R. and Parsons, S. G. (2010) The mass of the white dwarf in GW Libra. Astrophysical Journal Letters, Vol.715 (No.2). L109-L112. doi:10.1088/2041-8205/715/2/L109

Preview

Text WRAP_Steeghs_GW_Libra_1004.3065v1 (2).pdf - Accepted Version Download (371Kb) | Preview

Request Changes to record.

Abstract

We report a mass and rotational broadening (v sin i) for the pulsating white dwarf (WD) component of the WZ Sge type Dwarf Nova GW Lib based on high-resolution Very Large Telescope spectroscopy that resolves the Mg II 4481 angstrom absorption feature. Its gravitational redshift combined with WD mass-radius models provides us with a direct measurement of the WD mass of M-1 = 0.84 +/- 0.02 M-circle dot. The line is clearly resolved and if associated with rotational broadening gives v sin i = 87.0 +/- 3.4 km s(-1), equivalent to a spin period of 97 +/- 12 s.

Item Type:	Journal Article
Subjects:	Q Science > QB Astronomy
Divisions:	Faculty of Science > Physics
Library of Congress Subject Headings (LCSH):	White dwarf stars, Cataclysmic variable stars
Journal or Publication Title:	Astrophysical Journal Letters
Publisher:	IOP Publishing Ltd
ISSN:	2041-8205
Official Date:	1 June 2010
Dates:	Date Event 1 June 2010 Published
Date of first compliant deposit:	3 December 2015
Date of first compliant Open Access:	3 December 2015
Volume:	Vol.715
Number:	No.2
Number of Pages:	4
Page Range:	L109-L112
DOI:	10.1088/2041-8205/715/2/L109
Status:	Peer Reviewed
Publication Status:	Published
Access rights to Published version:	Restricted or Subscription Access
Funder:	Science and Technology Facilities Council (Great Britain) (STFC)
Related URLs:	Other Repository

Data sourced from Thomson Reuters' Web of Knowledge

Request changes or add full text files to a record

Repository staff actions (login required)

View Item

Downloads