Spectroscopy of novae and supernovae

Details Spectroscopy of novae and supernovae Spectroscopy of novae and supernovae

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993basi...21..255p&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 21, no. 3-4, p. 255-265

Astronomy and Astrophysics

Astronomy

1

Astronomical Spectroscopy, Novae, Spectrophotometry, Supernovae, Balmer Series, Data Correlation, H Alpha Line, H Beta Line, Spectrum Analysis

Scientific paper

Many novae have been studied spectroscopically since 1975 and many supernovae since 1980 using the telescopes at Vainu Bappu Observatory (VBO). The program on novae has intensified since 1985, and that on supernovae has found renewed interest since SN 1987A. The availability of the CCD detector in 1989 and of the Boller & Chivens spectrograph at the Vainu Bappu Telescope (VBT) in 1991 have added impetus to these studies. The motivation for these studies are summarized in this review together with some of the important results obtained with the VBT. The desirable improvements at the VBT are summarized at the end.

Affiliated with

Also associated with

No associations

Rating

Spectroscopy of novae and supernovae 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 Spectroscopy of novae and supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopy of novae and supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1561494