Nebular Phase Synthetic Spectra of SN1993J

Details Nebular Phase Synthetic Spectra of SN1993J Nebular Phase Synthetic Spectra of SN1993J

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...183.3905h&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #39.05; Bulletin of the American Astronomical Society, Vol. 25, p.1349

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Using a helium star explosion model from Nomoto et al. (1993), we construct non-LTE synthetic spectra for SN1993J for a number of epochs later than 100 days. In the spectrum calculation, line transfer is treated in the Sobolev approximation and explicitly includes non-local radiative coupling. Nonthermal energy deposition from (56) Co decay is treated by solving the Boltzman equation; excitation, ionization and thermal equilibrium are solved self consistently. We compare our synthetic spectra with RGO archive data from recent WHT spectral observations of SN1993J. In particular, we investigate the spectroscopic effects of mixing in the ejecta by comparing synthetic spectra of macroscopically mixed models with the observed spectra.

Affiliated with

Also associated with

No associations

Rating

Nebular Phase Synthetic Spectra of SN1993J 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 Nebular Phase Synthetic Spectra of SN1993J, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nebular Phase Synthetic Spectra of SN1993J will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-778512