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A radial velocity study of CTCV J1300−3052
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Savoury, C. D. J., Littlefair, S. P., Marsh, T. R., Dhillon, V. S., Parsons, S. G., Copperwheat, C. M. and Steeghs, D. (Danny), 1972-. (2012) A radial velocity study of CTCV J1300−3052. Monthly Notices of the Royal Astronomical Society, Vol.422 (No.1). pp. 469-477. ISSN 00358711
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WRAP_Steeghs_1201.4977v1.pdf - Accepted Version Restricted to Repository staff only until 13 September 2012. Download (1021Kb) |
Official URL: http://dx.doi.org/10.1111/j.1365-2966.2012.20625.x
Abstract
We present time-resolved spectroscopy of the eclipsing, short-period cataclysmic variable CTCV J1300−3052. Using absorption features from the secondary star, we determine the radial velocity semi-amplitude of the secondary star to be K2= 378 ± 6 km s−1, and its projected rotational velocity to be v sin i= 125 ± 7 km s−1. Using these parameters and Monte Carlo techniques, we obtain masses of M1= 0.79 ± 0.05 M⊙ for the white dwarf primary and M2= 0.198 ± 0.029 M⊙ for the M-type secondary star. These parameters are found to be in good agreement with previous mass determinations found via photometric fitting techniques, supporting the accuracy and validity of photometric mass determinations in short-period CVs.
| Item Type: | Journal Article |
|---|---|
| Subjects: | Q Science > QB Astronomy |
| Divisions: | Faculty of Science > Physics |
| Library of Congress Subject Headings (LCSH): | Cataclysmic variable stars |
| Journal or Publication Title: | Monthly Notices of the Royal Astronomical Society |
| Publisher: | John Wiley & Sons Ltd. |
| ISSN: | 00358711 |
| Date: | 2012 |
| Volume: | Vol.422 |
| Number: | No.1 |
| Page Range: | pp. 469-477 |
| Identification Number: | 10.1111/j.1365-2966.2012.20625.x |
| Status: | Peer Reviewed |
| Publication Status: | Published |
| Access rights to Published version: | Restricted or Subscription Access |
| Funder: | Science and Technology Facilities Council (Great Britain) (STFC), Research Councils UK (RCUK) |
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| URI: | http://wrap.warwick.ac.uk/id/eprint/45921 |
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