The early spectroscopy of V2670 Oph (Nova Oph 2008)

Details The early spectroscopy of V2670 Oph (Nova Oph 2008) The early spectroscopy of V2670 Oph (Nova Oph 2008)

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ap%26ss.323..319p&link_type=abstract

Astrophysics and Space Science, Vol. 323, p. 319-322

Astronomy and Astrophysics

Astrophysics

Stars: Novae, Cataclysmic Variables

Scientific paper

We report the spectroscopic observations of nova V2670 Oph secured at the Loiano Observatory, Italy, 39 days after the outburst. The spectra of V2670 Oph showed auroral lines, suggesting that ionization was increasing. V2670 Oph is a fast nova, with a decline rate by three magnitudes of 42 days. We have estimated the absolute magnitude at maximum and the distance of V2670 Oph. The nova achieved an absolute magnitude at maximum in the interval -7.9,…,-7.4. The distance of V2670 Oph is in the range 4.7-5.8 kpc.

Affiliated with

Also associated with

No associations

Rating

The early spectroscopy of V2670 Oph (Nova Oph 2008) 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 The early spectroscopy of V2670 Oph (Nova Oph 2008), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The early spectroscopy of V2670 Oph (Nova Oph 2008) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-805139