Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.282.1211s&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 282, Issue 4, pp. 1211-1222.
Astronomy and Astrophysics
Astronomy
59
Novae, Cataclysmic Variables, Infrared: Stars
Scientific paper
We have measured J and K colours for a sample of 36 predominantly faint cataclysmic variables (CVs) at high Galactic latitude. The J-K colours lie blueward of the main sequence, consistent with moderate (~20 per cent) contamination of the secondary light by an accretion disc. We use the K magnitudes to estimate the distances of the stars. We show that most lie within about 400 pc, and only two of the stars in our sample (RU LMi and DO Leo) are convincingly at Galactic halo distances. We have determined M_V values based on quiescent V magnitudes. The long-period dwarf nova systems (P<~3h) have absolute magnitudes which are consistent with the previously observed range. However, for the short-period dwarf novae the range of M_V extends to much fainter magnitudes than previously believed (as faint as M_V=14). We find that those systems that have large outburst amplitudes tend to be those with the faintest M_Vs in quiescence.
Howell Steve B.
Mason Keith O.
Sproats L. N.
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