Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.265l..29w&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Vol. 265, NO. 3/DEC1, P. L29, 1993
Astronomy and Astrophysics
Astronomy
11
Accretion, Accretion Discs - Binaries: Close - Stars: Individual: V2009-65.5 - Stars: Magnetic Fields - Novae, Cataclysmic Variables
Scientific paper
Recently, Buckley et al. drew attention to a new AM Her variable, RE1938-4612 , discovered by the ROSAT survey with a period of 2.33 h which places it in the middle of the usual 2-3 h period gap for cataclysmic variables. Here, we report the discovery of yet another AM Her variable, V2009-65.5, with a period of 2.66 h, also within the period gap. We argue that the anomalously high proportion of AM Hers within the period gap indicates that the canonical magnetic braking mechanism used to explain the orbital evolution of other CVs may not be applicable to the AM Hers. Possible alternative models are discussed.
Bailey Jon A.
Dopita Mike A.
Drissen Laurent
Ferrario Lilia
Hough James H.
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