Detection of a periodicity from Classical Nova Cygni 2006 (V2362 Cygni) in the optical wavelengths

Details Detection of a periodicity from Classical Nova Cygni 2006 (V2362 Cygni) in the optical wavelengths Detection of a periodicity from Classical Nova Cygni 2006 (V2362 Cygni) in the optical wavelengths

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2137....1b&link_type=abstract

The Astronomer's Telegram, #2137

Astronomy and Astrophysics

Astronomy

1

Optical, Binaries, Cataclysmic Variables, Novae, Transients, Variables

Scientific paper

We obatined V band photometric data of the classical nova V2362 Cyg (Nova Cygni 2006) using a 30 cm Schmidt-Cassegrain telescope equipped with an ST-9XE CCD camera of the Cukurova University Observatory, Adana, Turkey. The CCD camera uses classical UBVRI Bessel filters. Our observations started on 12 Jun 2006 about 72 days after the maximum brightness and continued on several distinct nights through 2006 and 2007 for a total of 50 nights (35 nights in 2006 and 15 nights in 2007).

Affiliated with

Also associated with

No associations

Rating

Detection of a periodicity from Classical Nova Cygni 2006 (V2362 Cygni) in the optical wavelengths 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 Detection of a periodicity from Classical Nova Cygni 2006 (V2362 Cygni) in the optical wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of a periodicity from Classical Nova Cygni 2006 (V2362 Cygni) in the optical wavelengths will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1781528