ar X iv : a st ro - p h / 02 10 45 8 v 1 2 1 O ct 2 00 2 Nova Scorpii 1941 ( V 697 Sco ) : A Probable Intermediate Polar

نویسنده

  • Patrick A. Woudt
چکیده

V697 Sco, the remnant of Nova Scorpii 1941 and currently at V ∼ 20.0, is found from photometric observations to have the characteristics of an intermediate polar (IP) with an orbital period (Porb) of 4.49 h and a rotation period (Prot) of 3.31 h. It therefore appears to be a member of the rare class of IPs where Prot ∼ Porb, which are probably discless systems. The prominence of the modulation at 1 2 Prot, and its orbital sidebands, indicates two-pole accretion. Subject headings: cataclysmic variables, stars: binaries: close, star: individual (V697 Sco)

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تاریخ انتشار 2002