Search for radio emission of nova-like cataclysmic variables

Details Search for radio emission of nova-like cataclysmic variables Search for radio emission of nova-like cataclysmic variables

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007atnf.prop.1021k&link_type=abstract

ATNF proposal C1732, Semester: October, 2007

Computer Science

Stellar, Galactic, Atca

Scientific paper

We have recently detected radio emission from a dwarf-nova cataclysmic variable (CV) in outburst for the first time. The source was initially detected in the radio-band during the optical rise. This was followed by a radio flare and continuous weak radio emission during all of the optical outburst. The behaviour is similar to that seen in X-ray binaries. Here, we propose to observe two nova-like CVs. Compared to a dwarf-nova a nova-like star is constantly in outburst. As the accretion rate is the major difference between those source classes, nova-like objects should be persistend radio emitters, which should be detected in a 12h ATCA observation.

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