NSV 1436, listed in the New Catalogue of Suspected Variable Stars (NSV), is a cataclysmic variable star in the constellation Perseus. It is believed to be similar to a dwarf nova like the star U Geminorum, but little is known Read more
NSV 1436 was discovered in outburst by E. Muyllaert (Oostende, Belgium) at an unfiltered (CV) magnitude of 13.49 on 2011 March 28.9576 (JD2455649.4576), and was confirmed by M. Linnolt (Hawaii, United States) at a visual magnitude of 12.8 on March 30.2708 (JD 24556450.7708). This star last exhibited a bright outburst in late November 1948 (Brown et al., 2010, JAAVSO 38, 176), and is a known X-ray source (Bedient 2004, priv. comm.). A smaller outburst occurred on 2011 March 9-10, when it briefly reached magnitude ~14.5 (Linnolt: 14.5 on JD 2455629.7618; M. Simsonsen, Michigan, United States: V=14.55 on JD 2455630.6615; Linnolt: 14.55 on JD 2455630.7354).