Four X-ray-selected cataclysmic variables in the Galactic plane

Details Four X-ray-selected cataclysmic variables in the Galactic plane Four X-ray-selected cataclysmic variables in the Galactic plane

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...364..251h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 364, Nov. 20, 1990, p. 251-258. Research supported by the U.S. Navy.

Astronomy and Astrophysics

Astronomy

29

Cataclysmic Variables, Dwarf Novae, Sky Surveys (Astronomy), X Ray Astronomy, X Ray Binaries, Magnetic Stars, Stellar Luminosity, Stellar Magnitude, Stellar Mass Accretion, Stellar Spectrophotometry, Variable Stars

Scientific paper

Four X-ray sources from the Einstein Galactic Plane Survey are identified here with faint CVs. These CVs have apparent V magnitudes between 17.5 and 19, making them faint both optically and in X-rays compared with other CVs. One CV, 1E 0830.9 - 2238, is probably an AM Herculis-type magnetic variable. The other three CVs appear to be standard nonmagnetic CVs with very low accretion rates. It is suggested that low accretion rate CVs may be very common.

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