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

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...

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Autores principales: Giacani, E.B., Dubner, G., Cappa, C., Testori, J.
Formato: JOUR
Materias:
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_03650138_v133_n1_p61_Giacani
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spelling todo:paper_03650138_v133_n1_p61_Giacani2023-10-03T15:27:42Z The structure of atomic gas around the supernova remnant 3C 400.2 Giacani, E.B. Dubner, G. Cappa, C. Testori, J. ISM: structure Radio lines: ISM Supernova remnants (SNRs) Supernova remnants: individual (3C 400.2) 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 velocity range +14 to +42 km s-1, and high velocity clouds probably accelerated by the supernova blast wave at v = -49.5 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. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_03650138_v133_n1_p61_Giacani
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic ISM: structure
Radio lines: ISM
Supernova remnants (SNRs)
Supernova remnants: individual (3C 400.2)
spellingShingle ISM: structure
Radio lines: ISM
Supernova remnants (SNRs)
Supernova remnants: individual (3C 400.2)
Giacani, E.B.
Dubner, G.
Cappa, C.
Testori, J.
The structure of atomic gas around the supernova remnant 3C 400.2
topic_facet ISM: structure
Radio lines: ISM
Supernova remnants (SNRs)
Supernova remnants: individual (3C 400.2)
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 v = -49.5 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 JOUR
author Giacani, E.B.
Dubner, G.
Cappa, C.
Testori, J.
author_facet Giacani, E.B.
Dubner, G.
Cappa, C.
Testori, J.
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
url http://hdl.handle.net/20.500.12110/paper_03650138_v133_n1_p61_Giacani
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