1H 1933+510: not a nova-like variable, but a dwarf nova
C. Bryja reported that this variable, which was originally identified as
a nova-like, to be more than three magnitudes high on July 23.
S. O'Connor reported that it was at 15.8mag on July 24, and
confirmed the outburst (
vsnet-campaign 392,
vsnet-campaign 393,
vsnet-campaign 394). A rather hasty fade was reported on July 25
by S. O'Connor (16.5mag) (
vsnet-campaign 395,
vsnet-campaign 398). Another outburst was reported by S. O'Connor
at 15.8mag on August 4 (vsnet-campaign 408). T. Vanmunster performed
CCD photometry on August 04/05 and reported that the resulting light
curve shows some small modulations, but clearly nothing related to superhumps
(vsnet-campaign 411).
G. Tovmassian and S. Zharikov got the spectrum which looks very similar
to Dwarf Novae in outburst (
vsnet-campaign 413). S. O'Connor reported an outburst on August 18
in [vsnet-obs 29195]
(vsnet-campaign 430).