2A 0526-328 - an X-ray-emitting cataclysmic variable

Details 2A 0526-328 - an X-ray-emitting cataclysmic variable 2A 0526-328 - an X-ray-emitting cataclysmic variable

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231l.131c&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 231, Aug. 1, 1979, p. L131-L135.

Astronomy and Astrophysics

Astrophysics

28

Variable Stars, X Ray Sources, Emission Spectra, Line Spectra

Scientific paper

The weak hard X-ray source 2A 0526-328 is identified with a previously unknown cataclysmic variable on the basis of its optical emission-line spectrum and a precise X-ray location. This star has a V magnitude of about 11 and spectral properties similar to dwarf novae at minimum light and AM Her, but shows no polarization. It is likely to be a Z Camelopardalis-type system in a very extended standstill (i.e., 'novalike' or UX Ursae Majoris-type) or a recurrent nova that has not erupted in recent times.

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