Nova V2362 Cygni increases its brightness

Details Nova V2362 Cygni increases its brightness Nova V2362 Cygni increases its brightness

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006atel..928....1g&link_type=abstract

The Astronomer's Telegram, #928

Astronomy and Astrophysics

Astronomy

8

Optical, Binaries, Novae

Scientific paper

Classical nova V2362 Cyg (N Cyg 2006, 23:11:32.34, +44:48:03.9, 2000) undergoes gradual increase of its brightness since middle of August, 2006 from the level of V = 11.9. In October 27, 2006 it has reached V = 11.26. The rate of this brightening is rising during the last week. This development resembles the scenario of V1493 Aql with the large hump superimposed on the descending branch of the light curve.

Affiliated with

Also associated with

No associations

Rating

Nova V2362 Cygni increases its brightness does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Nova V2362 Cygni increases its brightness, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nova V2362 Cygni increases its brightness will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1311522