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The eclipsing intermediate polar V597 Pup (Nova Puppis 2007)
Authors:Brian Warner   Patrick A. Woudt
Affiliation:Department of Statistics, University of the Western Cape, Private Bag X17, Bellville, 7535 Cape, South Africa
Abstract:JL 82 is a known binary, consisting of an sdB star and a companion which is not directly observable in the optical. Photometric measurements reported in this paper show it to variable with both the binary period (∼0.75 d), as well as on much shorter time-scales. The shorter periods are ascribed to pulsation of the sdB star, making it a member of the PG 1716 class of pulsating stars.
Keywords:binaries: close    stars: individual: JL 82    stars: oscillations    subdwarfs    stars: variables: other
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