Kesao Takamizawa (Nagano, Japan) reports his discovery of a new large-amplitude variable star located at 22h 31m 14s.66 +06o 22' 49".0 (J2000.0). His photographic magnitude estimates:
Photographic magnitude estimates by VSOLJ members object YYMMDD(UT) mag code J223114+0622 940506.738 <155P Tmz.VSOLJ J223114+0622 940516.745 <155P Tmz.VSOLJ J223114+0622 940705.644 153P Tmz.VSOLJ J223114+0622 940810.682 121P Tmz.VSOLJ J223114+0622 940904.545 115P Tmz.VSOLJ J223114+0622 940930.615 120P Tmz.VSOLJ J223114+0622 941027.547 135P Tmz.VSOLJ J223114+0622 941124.488 <150P Tmz.VSOLJ J223114+0622 941221.435 <150P Tmz.VSOLJ J223114+0622 950426.769 119P Tmz.VSOLJ J223114+0622 950820.599 <154P Tmz.VSOLJ J223114+0622 960712.674 121P Tmz.VSOLJ
The object coincides with a 13.0-mag GSC star. The light variation suggests a Mira-type variable star with a period of ~7 months, although there is no corresponding object in the IRAS PSC (out of the scan area?).
Follow-up observations are encouraged during the present bright phase.
Regards,
Taichi Kato