Emisiones no térmicas en radiofuentes compactas

A formula for the X-ray flux from Compton-synchrotron emissivity is derived. The values of flux obtained for some radiosources taking the values of magnetic field derived from the assumption of equipartition of energy between the magnetic field and cosmic rays are well below the limits of sensitivit...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Terlevich, R., Frank, J., Albano, J. R.
Formato: Articulo Comunicacion
Lenguaje:Español
Publicado: 1980
Materias:
Astronomía
Galaxias
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/99325
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-99325
record_format dspace
spelling I19-R120-10915-993252024-09-11T19:01:55Z http://sedici.unlp.edu.ar/handle/10915/99325 Emisiones no térmicas en radiofuentes compactas Terlevich, R. Frank, J. Albano, J. R. 1980 2020-06-29T12:10:50Z es Astronomía Galaxias A formula for the X-ray flux from Compton-synchrotron emissivity is derived. The values of flux obtained for some radiosources taking the values of magnetic field derived from the assumption of equipartition of energy between the magnetic field and cosmic rays are well below the limits of sensitivity reached by recent measurements. However if the magnetic field is derived from the synchrotron auto-absorption theory, the values of the predicted flux are 103 larger and they could be detected. Asociación Argentina de Astronomía Articulo Comunicacion http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Astronomía
Galaxias
spellingShingle Astronomía
Galaxias
Terlevich, R.
Frank, J.
Albano, J. R.
Emisiones no térmicas en radiofuentes compactas
topic_facet Astronomía
Galaxias
description A formula for the X-ray flux from Compton-synchrotron emissivity is derived. The values of flux obtained for some radiosources taking the values of magnetic field derived from the assumption of equipartition of energy between the magnetic field and cosmic rays are well below the limits of sensitivity reached by recent measurements. However if the magnetic field is derived from the synchrotron auto-absorption theory, the values of the predicted flux are 103 larger and they could be detected.
format Articulo
Comunicacion
author Terlevich, R.
Frank, J.
Albano, J. R.
author_facet Terlevich, R.
Frank, J.
Albano, J. R.
author_sort Terlevich, R.
title Emisiones no térmicas en radiofuentes compactas
title_short Emisiones no térmicas en radiofuentes compactas
title_full Emisiones no térmicas en radiofuentes compactas
title_fullStr Emisiones no térmicas en radiofuentes compactas
title_full_unstemmed Emisiones no térmicas en radiofuentes compactas
title_sort emisiones no térmicas en radiofuentes compactas
publishDate 1980
url http://sedici.unlp.edu.ar/handle/10915/99325
work_keys_str_mv AT terlevichr emisionesnotermicasenradiofuentescompactas
AT frankj emisionesnotermicasenradiofuentescompactas
AT albanojr emisionesnotermicasenradiofuentescompactas
_version_ 1823259468759040000

Ejemplares similares