Infrared Photometry and Spectroscopy of Nova Pw-Vulpecuale

Details Infrared Photometry and Spectroscopy of Nova Pw-Vulpecuale Infrared Photometry and Spectroscopy of Nova Pw-Vulpecuale

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.246..527e&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 246, NO. 3/OCT1, P. 527, 1990

Astronomy and Astrophysics

Astronomy

16

Scientific paper

We present near-infrared photometry and spectroscopy of the slow nova PW Vul (Nova Vul 1984 No. 1) prior to its dust-formation phase. In common with the visual light curve, the near-infrared light curves varied extremely erratically during the first 100 d after maximum. Emission lines of C and N were prominent in the near-infrared spectra, as would be expected from the thermonuclear-runaway model of the nova outburst, but He I lines were weak. A distance of 3 kpc is consistent with a number of independent distance indicators.

Affiliated with

Also associated with

No associations

Rating

Infrared Photometry and Spectroscopy of Nova Pw-Vulpecuale 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 Infrared Photometry and Spectroscopy of Nova Pw-Vulpecuale, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Infrared Photometry and Spectroscopy of Nova Pw-Vulpecuale will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1304713