We present time-resolved J-band spectroscopy of the short-period cataclysmic variable SDSS J143317.78+101123.3. We detect absorption lines from the sub-stellar donor star in this system, which contributes 38 +/- 5 per cent to the J-band light. From the relative strengths of the absorption lines in the J band, we estimate the spectral type of the donor star to be L2 +/- 1. These data are the first spectroscopic detection of a donor with a confirmed sub-stellar mass in a cataclysmic variable, and the spectral type is consistent with that expected from semi-empirical evolutionary models.
Using skew mapping, we have been able to derive an estimate for the radial velocity of the donor of K-d = 520 +/- 60 km/s. This value is consistent with, though much less precise than, predictions from mass determinations found via photometric fitting of the eclipse light curves.
|Journal||Monthly Notices of the Royal Astronomical Society|
|Publication status||Published - 26 Mar 2013|
- binaries: eclipsing
- stars: dwarf novae
- stars: individual: SDSS J1433+1011
- novae, cataclysmic variables
- PERIOD CATACLYSMIC VARIABLES
- DWARF LIKE SECONDARIES