This variable star was last year discovered in a bright state by K. Takamizawa. We have not yet heard further information of this object since. Follow-up observations during this favorabale season are still encouraged. ---------------------------------------------------------------------- (from vsnet-alert 92, 1995 Mar. 31) | Subject: [vsnet-alert 92] brightening of NSV06481 | | K. Takamizawa (Nagano, Japan) reports his photographic discovery of | a brightening of NSV 06481. The original observations follow: | | object YYMMDD(UT) mag code | NSV06481 940506.595 141P K.Takamizawa | NSV06481 950328.660 124P K.Takamizawa | | Instruments: 10-cm refr. (fl=400mm) photographic. T-Max 400 | | M. Iida (Nagano, Japan) further reports that NSV 06481 is cataloged | in NSV as a suspected variable star with a range of 14.5 - [15.5 p, type | unknown. The object is not registered in IRAS PSC. Hence NSV 06481 seems | less likely to be identified as a red variable. | | M. Iida further provides his survey of photographic atlases: | | Vehrenberg: fainter than 15.4 | Lick: 14.5: | GSC: 14.9 | | An examination of a photograph by K. Takamizawa confirms an identification | of NSV 06481 with a GSC star (V=14.9) at the corresponding position. | | Although the materials have not been conclusive, M. Iida suspects this | object to be a some sort of eruptive or cataclysmic variable. Follow-up | observations are urgently needed. Spectroscopic observations and multicolor | photometry would be most helpful. | | Regards, | Taichi Kato ---------------------------------------------------------------------- (from vsnet-alert 93, 1995 Mar. 31) | Subject: [vsnet-alert 93] position of NSV06481 | | NSV06481 | | M. Iida further provides the following accurate position of the object | in question. | | 13h 53m 32s.74 -29o 05' 42".0 (J2000.0) from GSC | | Taichi Kato ----------------------------------------------------------------------