Modeling the early spectra of SN 1993J using the Monte Carlo method.

Details Modeling the early spectra of SN 1993J using the Monte Carlo method. Modeling the early spectra of SN 1993J using the Monte Carlo method.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..355l&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 4, p. 355 - 364

Astronomy and Astrophysics

Astrophysics

Supernovae: Spectra, Supernovae: Stellar Atmospheres

Scientific paper

This paper describes how to apply the Monte Carlo method to model the early spectra of supernovae (SNe). By dividing the total energy radiated from the photosphere of SNe into a lot of photon packages and then tracing the movement of these packages, this method can solve the line overlapping problem of supernova spectrum simulations. Programs to construct density profiles and abundance structures of supernova envelopes and to compare the model with the observation are compiled, which makes the Monte Carlo-spectrum-synthesis software package well adapted to modeling the early spectra of SNe. The authors present an example of modeling the 1993 April 13 spectrum of SN 1993J.

Affiliated with

Also associated with

No associations

Rating

Modeling the early spectra of SN 1993J using the Monte Carlo method. 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 Modeling the early spectra of SN 1993J using the Monte Carlo method., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Modeling the early spectra of SN 1993J using the Monte Carlo method. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1212087