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Infrared Properties of Cataclysmic Variables from 2MASS: Results from the 2nd Incremental Data Release

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arxiv astro-ph/0109393 v1 pith:6DKVLJEQ submitted 2001-09-21 astro-ph

Infrared Properties of Cataclysmic Variables from 2MASS: Results from the 2nd Incremental Data Release

D. W. Hoard (1) , S. Wachter (1) , L. Lee Clark (2) , Timothy P. Bowers (3) ((1) Cerro Tololo Inter-American Observatory , (2) San Diego State University , (3) Steward Observatory/University of Arizona) This is my paper
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keywords cataclysmicvariablesdataincrementalinfraredmassnear-irphotometry
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Because accretion-generated luminosity dominates the radiated energy of most cataclysmic variables, they have been ``traditionally'' observed primarily at short wavelengths. Infrared observations of cataclysmic variables contribute to the understanding of key system components that are expected to radiate at these wavelengths, such as the cool outer disk, accretion stream, and secondary star. We have compiled the J, H, and Ks photometry of all cataclysmic variables located in the sky coverage of the 2 Micron All Sky Survey (2MASS) 2nd Incremental Data Release. This data comprises 251 systems with reliably identified near-IR counterparts and S/N > 10 photometry in one or more of the three near-IR bands.

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  1. SRG/eROSITA X-ray selected cataclysmic variable candidates observed in SDSS-V DR20

    astro-ph.SR 2026-07 conditional novelty 6.0

    eROSITA-selected SDSS-V DR20 spectroscopy yields 587 cataclysmic variables (274 known), including new nearby systems, AM CVns, and a low-accretion-rate polar.