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).

Light Curve and General Information of This Object