The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3

The results of a new high-resolution study of the molecular gas associated with the supernova remnants (SNR) G349.7+G18.8+0.3 were presented. The observations were performed with the SEST telescope in the 12Co J= 1-0, 2-1 and 3-2 lines. The observations have provided the new evidence in support to t...

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Guardado en:
Detalles Bibliográficos
Publicado: 2004
Materias:
ISM: clouds
ISM: molecules
ISM: supernova remnants
Radio lines: ISM
Interstellar medium (ISM)
Molecular clouds
Supernova remnants (SNR)
X-ray emission
Clouds
Light emission
Masers
Morphology
Radio communication
Radio telescopes
X rays
Astrophysics
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v426_n1_p201_Dubner
http://hdl.handle.net/20.500.12110/paper_00046361_v426_n1_p201_Dubner
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires
id paper:paper_00046361_v426_n1_p201_Dubner
record_format dspace
spelling paper:paper_00046361_v426_n1_p201_Dubner2023-06-08T14:27:35Z The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3 ISM: clouds ISM: molecules ISM: supernova remnants Radio lines: ISM Interstellar medium (ISM) Molecular clouds Supernova remnants (SNR) X-ray emission Clouds Light emission Masers Morphology Radio communication Radio telescopes X rays Astrophysics The results of a new high-resolution study of the molecular gas associated with the supernova remnants (SNR) G349.7+G18.8+0.3 were presented. The observations were performed with the SEST telescope in the 12Co J= 1-0, 2-1 and 3-2 lines. The observations have provided the new evidence in support to the existence of physical interaction between the SN shocks and the adjoining molecular clouds, for the two SNRs. It was concluded that the masers were excited at the sites where a non-dissociative C-type shock, locally transverse to the line of sight, hits a denser molecular clump. 2004 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v426_n1_p201_Dubner http://hdl.handle.net/20.500.12110/paper_00046361_v426_n1_p201_Dubner
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: clouds
ISM: molecules
ISM: supernova remnants
Radio lines: ISM
Interstellar medium (ISM)
Molecular clouds
Supernova remnants (SNR)
X-ray emission
Clouds
Light emission
Masers
Morphology
Radio communication
Radio telescopes
X rays
Astrophysics
spellingShingle ISM: clouds
ISM: molecules
ISM: supernova remnants
Radio lines: ISM
Interstellar medium (ISM)
Molecular clouds
Supernova remnants (SNR)
X-ray emission
Clouds
Light emission
Masers
Morphology
Radio communication
Radio telescopes
X rays
Astrophysics
The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
topic_facet ISM: clouds
ISM: molecules
ISM: supernova remnants
Radio lines: ISM
Interstellar medium (ISM)
Molecular clouds
Supernova remnants (SNR)
X-ray emission
Clouds
Light emission
Masers
Morphology
Radio communication
Radio telescopes
X rays
Astrophysics
description The results of a new high-resolution study of the molecular gas associated with the supernova remnants (SNR) G349.7+G18.8+0.3 were presented. The observations were performed with the SEST telescope in the 12Co J= 1-0, 2-1 and 3-2 lines. The observations have provided the new evidence in support to the existence of physical interaction between the SN shocks and the adjoining molecular clouds, for the two SNRs. It was concluded that the masers were excited at the sites where a non-dissociative C-type shock, locally transverse to the line of sight, hits a denser molecular clump.
title The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
title_short The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
title_full The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
title_fullStr The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
title_full_unstemmed The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
title_sort molecular clouds in the environs of the supernova remnants g349.7+0.2 and g18.8+0.3
publishDate 2004
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v426_n1_p201_Dubner
http://hdl.handle.net/20.500.12110/paper_00046361_v426_n1_p201_Dubner
_version_ 1768543256718606336

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