HadV106
K. Haseda reported the discovery of a new variable star, named HadV106.
The object was reported to be fading to <13p mag in 2002 July. The
similar fading trend was also detected by A. Takao. Although the amplitude
and the IRAS flux may suggest a Mira-type variable, the object may have
been systematically bright before 2001. The fading in July therefore may
be a temporary one rather than a result of pulsation (vsnet-campaign-unknown
90, 93,
94).