The spectrum and evolution of compact SNR: SN and AGN.
Abstract
The evolution and spectra from a compact supernova remnant evolving in a high-density circumstellar medium with a density of 107cm-3 are presented. The radiation emitted by the shocked region can self-ionize the cooling shell and a large region of the surrounding medium. The resulting line ratios from the photoionized zones are similar to those observed in active galactic nuclei.
- Publication:
-
Revista Mexicana de Astronomia y Astrofisica
- Pub Date:
- November 1993
- Bibcode:
- 1993RMxAA..27..133F
- Keywords:
-
- Supernova Remnants: Synthetic Spectra;
- Supernova Remnants: Evolution;
- Supernova Remnants: Active Galactic Nuclei