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Dynamical masses of a nova-like variable on the edge of the period gap

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Rodríguez-Gil, P., Shahbaz, T., Marsh, Tom, Gänsicke, B. T. (Boris T.), Steeghs, D., Long, K. S., Martínez-Pais, I. G., Armas Padilla, M., Schwarz, R., Schreiber, M. R., Torres, M. A. P., Koester, D., Dhillon, V. S., Castellano, J. and Rodríguez, D. (2015) Dynamical masses of a nova-like variable on the edge of the period gap. Monthly Notices of the Royal Astronomical Society, 452 (1). pp. 146-157. doi:10.1093/mnras/stv1244 ISSN 0035-8711.

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Official URL: http://dx.doi.org/10.1093/mnras/stv1244

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Abstract

We present the first dynamical determination of the binary parameters of an eclipsing SW Sextantis star in the 3–4 h orbital period range during a low state. We obtained time-resolved optical spectroscopy and photometry of HS 0220+0603 during its 2004–2005 low-brightness state, as revealed in the combined Small & Moderate Aperture Research Telescope System, IAC80 and M1 Group long-term optical light curve. The optical spectra taken during primary eclipse reveal a secondary star spectral type of M5.5 ± 0.5 as derived from molecular band-head indices. The spectra also provide the first detection of a DAB white dwarf in a cataclysmic variable. By modelling its optical spectrum we estimate a white dwarf temperature of 30 000 ± 5000 K. By combining the results of modelling the white dwarf eclipse from ULTRACAM light curves with those obtained by simultaneously fitting the emission- and absorption-line radial velocity curves and I-band ellipsoidal light curves, we measure the stellar masses to be M1 = 0.87 ± 0.09 M⊙ and M2 = 0.47 ± 0.05 M⊙ for the white dwarf and the M dwarf, respectively, and an inclination of the orbital plane of i ≈ 79°. A radius of 0.0103 ± 0.0007 R⊙ is obtained for the white dwarf. The secondary star in HS 0220+0603 is likely too cool and undersized for its mass.

Item Type: Journal Article
Divisions: Faculty of Science, Engineering and Medicine > Science > Physics
Journal or Publication Title: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press
ISSN: 0035-8711
Official Date: 1 September 2015
Dates:
DateEvent
1 September 2015Published
1 June 2015Accepted
Volume: 452
Number: 1
Page Range: pp. 146-157
DOI: 10.1093/mnras/stv1244
Status: Peer Reviewed
Publication Status: Published
Access rights to Published version: Restricted or Subscription Access

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