V382 Vel
A possible variability was noticed in
[vsnet-campaign-nova 21],
however, M. Morel
(vsnet-campaign-nova 23)
and B. Monard
(vsnet-campaign-nova 24)
commented that there must be a difference
in the sequence used among observers. A. Retter additionally commented
that the nova, still bright at mV=10.5-11.0 was a very promising object
to search for periodicities even if the apparent oscillation was
spurious
(vsnet-campaign-nova 28).
S. Otero suggested that GSC 8210-00897 is the most suitable comparison
star
(vsnet-campaign-nova 29).