The structure of atomic gas around the supernova remnant 3C 400.2

Mostrar todas las versiones(2)

The interaction of the SNR 3C 400.2 with the interstellar medium is investigated on the basis of the HI observations using the Synthesis Radio Telescope at the Dominion Radio Astrophysical Observatory (DRAO). These new data show the existence of a dense atomic cloud associated with 3C 400.2 in the v...

Descripción completa

Detalles Bibliográficos
Autores principales: Giacani, E. B., Dubner, G. M., Cappa, Cristina Elisabet, Testori, Juan Carlos
Formato: Articulo
Lenguaje:Español
Publicado: 1998
Materias:
Ciencias Astronómicas
supernova remnants (SNRs)
supernova remnants: individual (3C 400.2)
radio lines: ISM
ISM: structure
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/123582
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-123582
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Español
topic Ciencias Astronómicas
supernova remnants (SNRs)
supernova remnants: individual (3C 400.2)
radio lines: ISM
ISM: structure
spellingShingle Ciencias Astronómicas
supernova remnants (SNRs)
supernova remnants: individual (3C 400.2)
radio lines: ISM
ISM: structure
Giacani, E. B.
Dubner, G. M.
Cappa, Cristina Elisabet
Testori, Juan Carlos
The structure of atomic gas around the supernova remnant 3C 400.2
topic_facet Ciencias Astronómicas
supernova remnants (SNRs)
supernova remnants: individual (3C 400.2)
radio lines: ISM
ISM: structure
description The interaction of the SNR 3C 400.2 with the interstellar medium is investigated on the basis of the HI observations using the Synthesis Radio Telescope at the Dominion Radio Astrophysical Observatory (DRAO). These new data show the existence of a dense atomic cloud associated with 3C 400.2 in the velocity range +14 to +42 km s -1 , and high velocity clouds probably accelerated by the supernova blast wave at  km s -1 and +69 km s -1 . We propose that the complex remnant 3C 400.2 is the result of a supernova explosion in a region of the interstellar medium containing a density discontinuity. A breakout phenomenon may explain the observed morphology in the different spectral regimes.
format Articulo
Articulo
author Giacani, E. B.
Dubner, G. M.
Cappa, Cristina Elisabet
Testori, Juan Carlos
author_facet Giacani, E. B.
Dubner, G. M.
Cappa, Cristina Elisabet
Testori, Juan Carlos
author_sort Giacani, E. B.
title The structure of atomic gas around the supernova remnant 3C 400.2
title_short The structure of atomic gas around the supernova remnant 3C 400.2
title_full The structure of atomic gas around the supernova remnant 3C 400.2
title_fullStr The structure of atomic gas around the supernova remnant 3C 400.2
title_full_unstemmed The structure of atomic gas around the supernova remnant 3C 400.2
title_sort structure of atomic gas around the supernova remnant 3c 400.2
publishDate 1998
url http://sedici.unlp.edu.ar/handle/10915/123582
work_keys_str_mv AT giacanieb thestructureofatomicgasaroundthesupernovaremnant3c4002
AT dubnergm thestructureofatomicgasaroundthesupernovaremnant3c4002
AT cappacristinaelisabet thestructureofatomicgasaroundthesupernovaremnant3c4002
AT testorijuancarlos thestructureofatomicgasaroundthesupernovaremnant3c4002
AT giacanieb structureofatomicgasaroundthesupernovaremnant3c4002
AT dubnergm structureofatomicgasaroundthesupernovaremnant3c4002
AT cappacristinaelisabet structureofatomicgasaroundthesupernovaremnant3c4002
AT testorijuancarlos structureofatomicgasaroundthesupernovaremnant3c4002
bdutipo_str Repositorios
_version_ 1764820449824342017

Ejemplares similares