MisV1147
This new variable star has gradually brightened. The object reached
12.34mag on 2001 October 3 from about 13.4mag on 2000 October
(vsnet-campaign-unknown 1).
S. Yoshida reported the
gradual brightening has already started in 2000 October when
the object was faint reaching 13.50mag
(vsnet-campaign-unknown 2).
T. Kato commented that if the object is a pre-main sequence
emission-line star, the star may be an object belonging to a small
subclass with occasional fadings like WW Vul, BO Cep etc
(vsnet-campaign-unknown 3).