arXiv · astro-ph/0411158
A New Cataclysmic Variable in Hercules
Abstract
We present time-series observations, spectra and archival outburst data of a newly-discovered variable star in Hercules, Var Her 04. Its orbital period, mass ratio, and outburst amplitude resemble those of the UGWZ-type subclass of UGSU dwarf novae. However, its supercycle and outburst light curve defy classification as a clear UGWZ. Var Her 04 is most similar to the small group of possible hydrogen-burning ``period bouncers'', dwarf novae that have passed beyond the period minimum and returned.
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A. Price, B. Gary, J. Bedient, L. Cook, M. Templeton, C. Pullen, D. Starkey, T. Crawford, R. Corlan, S. Dvorak, K. Graham, R. Huziak, R. James, D. Messier, N. Quinn, D. Boyd, J. Blackwell, G. Walker, M. Mattei, D. Rodriguez, M. Simonsen, A. Henden, T. Vanmunster, P. Garnavich, J. Pittichova, T. Matheson, P. Challis, R. P. Kirshner, E. Adams, T. Harrison, M. D. Koppelman, G. E. Sarty, D. E. Mais. 2004-11-09. A New Cataclysmic Variable in Hercules. https://doi.org/10.1086/427272
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