Discovery of a high-amplitude variability of the SU UMa dwarf nova = 1RXS J105120.5+672550 in quiescence

Details Discovery of a high-amplitude variability of the SU UMa dwarf nova = 1RXS J105120.5+672550 in quiescence Discovery of a high-amplitude variability of the SU UMa dwarf nova = 1RXS J105120.5+672550 in quiescence

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012atel.3889....1p&link_type=abstract

The Astronomer's Telegram, #3889

Astronomy and Astrophysics

Astronomy

Optical, Binary, Cataclysmic Variable, Star, Variables

Scientific paper

K. Sokolovsky and D. Denisenko detected a likely variable star during the search of new CVs from USNO-B1.0: Stars with Outbursts on IR Palomar Plates (cf. VSNET-alert 14060; arxiv:1108.5122). An outburst of this object was independently discovered by MASTER-Amur auto-detection system (MASTER OT105123.02+672528.3, (Atel #3845)) at V=14.6 mag and CATALINA robotic telescope (CSS120101:105123+672528, Drake et al., 2009, ApJ 696, 870) at 15.1 mag , VSNET alert 14055).Its quiescent magnitude is about 18.5 - 19 (VSNET-alert 3845, VSNET-alert 14060).

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