Time-resolved Photometry of the Recently-discovered SU UMa Star, OT J011306.7+215250

Details Time-resolved Photometry of the Recently-discovered SU UMa Star, OT J011306.7+215250 Time-resolved Photometry of the Recently-discovered SU UMa Star, OT J011306.7+215250

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008atel.1757....1s&link_type=abstract

The Astronomer's Telegram, #1757

Astronomy and Astrophysics

Astronomy

Optical, Cataclysmic Variables, Transients

Scientific paper

We report the results of time-resolved CCD photometry obtained with the Mount Laguna Observatory 1-m reflector of the SU UMa star OT J011306.7+215250, which was discovered on 2008 Sep 22 UT by Drake et al. (ATel #1734) as part of the Catalina Real-time Transient Survey. A total of ~25 hours of V-band photometry over 5 nights (2008 Sep 25 - 29 UT) has enabled us to confirm its SU UMa nature, and to establish a revised superhump period of 0.09445(3) days (136.0 minutes), which is one of the longest superhump periods known.

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