Superhumps in The Helium Dwarf Nova KL Draconis

Details Superhumps in The Helium Dwarf Nova KL Draconis Superhumps in The Helium Dwarf Nova KL Draconis

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...19915508w&link_type=abstract

American Astronomical Society, 199th AAS Meeting, #155.08; Bulletin of the American Astronomical Society, Vol. 34, p.562

Astronomy and Astrophysics

Astronomy

Scientific paper

We report on the discovery of a 25.5-minute superhump period for the suspected helium dwarf nova system KL Draconis in high state. The presence of superhumps combined with the previously-observed helium spectrum and large-amplitude photometric variations confirm that KL Dra is an AM CVn system similar to CR Bootis and CP Eridani. We gratefully acknowledge support from the National Science Foundation through the Research Experiences for Undergraduates Summer Site Program through grants AST-0097616 to Florida Tech and PHY-9531383 to Notre Dame.

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