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HS 2237+8154: A New Pre-CV just above the Period Gap
Published online by Cambridge University Press: 22 February 2018
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We report follow-up observations of the new pre-cataclysmic variable HS 2237+8154, identified from the Hamburg Quasar Survey. The orbital period derived from ellipsoidal modulation observed in the iR-band as well as from the Hα radial velocity variation is orb = 178.10 ± 0.08 min. We briefly discuss the evolutionary state of this system.
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- Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004
References
Araujo-Betancor, S., Gänsicke, B. Т., Ilagen, H.-J., Rodriguez-Gil, Р., & Engels, D.
2003, A&A, 406, 213
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Gänsicke, B. Т., Hagen, H. J., & Engels, D.
2002, in The Physics of Cataclysmic Variables and Related Objects, ed. Gänsicke, B. Т., Beuermann, K., & Reinsch, K. (ASP Conf. Ser. 261), 190, 199
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