Model for Synchrotron Emission from Shell Supernova Remnants in Nonuniform Interstellar Medium and Nonuniform Magnetic Field
| dc.creator | Petruk, O. | |
| dc.date | 2002-06-27 | |
| dc.date.accessioned | 2026-07-07T02:04:05Z | |
| dc.date.available | 2026-07-07T02:04:05Z | |
| dc.description | Possibility to model the high energy synchrotron emission (in X- and gamma-rays) from supernova remnants is an important task for modern astronomy and astrophysics, because it may be responsible for the nonthermal X-rays and TeV gamma-rays observed recently from a number of SNRs. This emission allows as to look in the processes of particle acceleration on SNR shocks and generation of cosmic rays. In this paper, a model for the synchrotron emission from shell SNR in nonuniform interstellar medium and nonuniform magnetic field is presented. This model is a generalization of the model of Reynolds and Chevalier developed for a spherical SNR in the uniform medium and uniform magnetic field. The model will be used for studies on the thermal and nonthermal X-ray images and spectra from nonspherical SNRs in different interstellar magnetic field configurations. | |
| dc.description | 6 pages. Contribution to the conference "Selected tasks in Astronomy and Astrophysics" (Lviv, April 2002) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0206484 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0206484 | |
| dc.identifier | J.Phys.Stud. 6 (2002) 401-403 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4615 | |
| dc.subject | Astrophysics | |
| dc.title | Model for Synchrotron Emission from Shell Supernova Remnants in Nonuniform Interstellar Medium and Nonuniform Magnetic Field | |
| dc.type | text |