Novalike variable MV Lyr: the results of a photometric multilongitude campaign

Details Novalike variable MV Lyr: the results of a photometric multilongitude campaign Novalike variable MV Lyr: the results of a photometric multilongitude campaign

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..393k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 393-396

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Scientific paper

The cataclysmic variable MV Lyr is nova-like variable, or ``anti-dwarf nova''. In 1979-1989 years this star similar to other ``anti-dwarf novae'' spent its time in a high brightness state (B≃ 12.5m) getting fainter by 2m-8m sometimes and returning to the ``on'' stage. But later its behaviour became non-typical for these stars. The length of its first deep minimum was 10 years. The~modern state is characterized by very strong outbursts and very frequent changes of the stages. The periods 0.128d and 0.136d were obtained for 1998 and 1999, respectively. We conclude about a~possible relation between the photometric period and brightness.

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