Natal molecular cloud of SNR Kes 41. Complete characterisation

Autores
Supán, Jorge Leonardo; Castelletti, Gabriela Marta; Supanitsky, Alberto Daniel; Burton, M.G; Wong, G.F.; Braiding, C.
Año de publicación
2018
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Using high-resolution data of the 12CO and 13CO (J = 1-0) line emission from the Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observations from the Southern Galactic Plane Survey (SGPS) and mid-infrared Spitzer data, we have explored the large-scale environment of the supernova remnant Kes 41. On the basis of these data, we identified for the first time the parent cloud of Kes 41 in its whole extension and surveyed the HII regions, masers, and the population of massive young stellar objects in the cloud. The whole unveiled giant cloud, located at the kinematic distance of 12.0 ± 3.6 kpc, whose average total mass and size are ~10-30 × 105 M and ∼ 26′, also shines in γ-rays, as revealed by the Large Area Telescope on board the Fermi satellite. We determined a high average proton density ∼500-1000 cm-3 in the large molecular complex, of which protons from the neutral atomic and ionised gases comprise only ∼15%.
Fil: Supán, Jorge Leonardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Castelletti, Gabriela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Burton, M.G. Armagh Observatory and Planetarium; Reino Unido. University of New South Wales. Faculty of Science; Australia
Fil: Wong, G.F.. University of New South Wales. Faculty of Science; Australia. Western Sydney University; Australia
Fil: Braiding, C.. University of New South Wales. Faculty of Science; Australia
Materia
GAMMA RAYS: ISM
ISM: INDIVIDUAL OBJECTS: KES 41
ISM: SUPERNOVA REMNANTS
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/97565
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/97565
network_acronym_str CONICETDig
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network_name_str CONICET Digital (CONICET)
spelling Natal molecular cloud of SNR Kes 41. Complete characterisationSupán, Jorge LeonardoCastelletti, Gabriela MartaSupanitsky, Alberto DanielBurton, M.GWong, G.F.Braiding, C.GAMMA RAYS: ISMISM: INDIVIDUAL OBJECTS: KES 41ISM: SUPERNOVA REMNANTShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Using high-resolution data of the 12CO and 13CO (J = 1-0) line emission from the Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observations from the Southern Galactic Plane Survey (SGPS) and mid-infrared Spitzer data, we have explored the large-scale environment of the supernova remnant Kes 41. On the basis of these data, we identified for the first time the parent cloud of Kes 41 in its whole extension and surveyed the HII regions, masers, and the population of massive young stellar objects in the cloud. The whole unveiled giant cloud, located at the kinematic distance of 12.0 ± 3.6 kpc, whose average total mass and size are ~10-30 × 105 M and ∼ 26′, also shines in γ-rays, as revealed by the Large Area Telescope on board the Fermi satellite. We determined a high average proton density ∼500-1000 cm-3 in the large molecular complex, of which protons from the neutral atomic and ionised gases comprise only ∼15%.Fil: Supán, Jorge Leonardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Castelletti, Gabriela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Burton, M.G. Armagh Observatory and Planetarium; Reino Unido. University of New South Wales. Faculty of Science; AustraliaFil: Wong, G.F.. University of New South Wales. Faculty of Science; Australia. Western Sydney University; AustraliaFil: Braiding, C.. University of New South Wales. Faculty of Science; AustraliaEDP Sciences2018-11info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/97565Supán, Jorge Leonardo; Castelletti, Gabriela Marta; Supanitsky, Alberto Daniel; Burton, M.G; Wong, G.F.; et al.; Natal molecular cloud of SNR Kes 41. Complete characterisation; EDP Sciences; Astronomy and Astrophysics; 619; 108; 11-2018; 1-70004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2018/11/aa33183-18/aa33183-18.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201833183info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:33:38Zoai:ri.conicet.gov.ar:11336/97565instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:33:38.782CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Natal molecular cloud of SNR Kes 41. Complete characterisation
title Natal molecular cloud of SNR Kes 41. Complete characterisation
spellingShingle Natal molecular cloud of SNR Kes 41. Complete characterisation
Supán, Jorge Leonardo
GAMMA RAYS: ISM
ISM: INDIVIDUAL OBJECTS: KES 41
ISM: SUPERNOVA REMNANTS
title_short Natal molecular cloud of SNR Kes 41. Complete characterisation
title_full Natal molecular cloud of SNR Kes 41. Complete characterisation
title_fullStr Natal molecular cloud of SNR Kes 41. Complete characterisation
title_full_unstemmed Natal molecular cloud of SNR Kes 41. Complete characterisation
title_sort Natal molecular cloud of SNR Kes 41. Complete characterisation
dc.creator.none.fl_str_mv Supán, Jorge Leonardo
Castelletti, Gabriela Marta
Supanitsky, Alberto Daniel
Burton, M.G
Wong, G.F.
Braiding, C.
author Supán, Jorge Leonardo
author_facet Supán, Jorge Leonardo
Castelletti, Gabriela Marta
Supanitsky, Alberto Daniel
Burton, M.G
Wong, G.F.
Braiding, C.
author_role author
author2 Castelletti, Gabriela Marta
Supanitsky, Alberto Daniel
Burton, M.G
Wong, G.F.
Braiding, C.
author2_role author
author
author
author
author
dc.subject.none.fl_str_mv GAMMA RAYS: ISM
ISM: INDIVIDUAL OBJECTS: KES 41
ISM: SUPERNOVA REMNANTS
topic GAMMA RAYS: ISM
ISM: INDIVIDUAL OBJECTS: KES 41
ISM: SUPERNOVA REMNANTS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Using high-resolution data of the 12CO and 13CO (J = 1-0) line emission from the Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observations from the Southern Galactic Plane Survey (SGPS) and mid-infrared Spitzer data, we have explored the large-scale environment of the supernova remnant Kes 41. On the basis of these data, we identified for the first time the parent cloud of Kes 41 in its whole extension and surveyed the HII regions, masers, and the population of massive young stellar objects in the cloud. The whole unveiled giant cloud, located at the kinematic distance of 12.0 ± 3.6 kpc, whose average total mass and size are ~10-30 × 105 M and ∼ 26′, also shines in γ-rays, as revealed by the Large Area Telescope on board the Fermi satellite. We determined a high average proton density ∼500-1000 cm-3 in the large molecular complex, of which protons from the neutral atomic and ionised gases comprise only ∼15%.
Fil: Supán, Jorge Leonardo. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Castelletti, Gabriela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Burton, M.G. Armagh Observatory and Planetarium; Reino Unido. University of New South Wales. Faculty of Science; Australia
Fil: Wong, G.F.. University of New South Wales. Faculty of Science; Australia. Western Sydney University; Australia
Fil: Braiding, C.. University of New South Wales. Faculty of Science; Australia
description Using high-resolution data of the 12CO and 13CO (J = 1-0) line emission from the Mopra Southern Galactic Plane CO Survey in conjunction with neutral hydrogen observations from the Southern Galactic Plane Survey (SGPS) and mid-infrared Spitzer data, we have explored the large-scale environment of the supernova remnant Kes 41. On the basis of these data, we identified for the first time the parent cloud of Kes 41 in its whole extension and surveyed the HII regions, masers, and the population of massive young stellar objects in the cloud. The whole unveiled giant cloud, located at the kinematic distance of 12.0 ± 3.6 kpc, whose average total mass and size are ~10-30 × 105 M and ∼ 26′, also shines in γ-rays, as revealed by the Large Area Telescope on board the Fermi satellite. We determined a high average proton density ∼500-1000 cm-3 in the large molecular complex, of which protons from the neutral atomic and ionised gases comprise only ∼15%.
publishDate 2018
dc.date.none.fl_str_mv 2018-11
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/97565
Supán, Jorge Leonardo; Castelletti, Gabriela Marta; Supanitsky, Alberto Daniel; Burton, M.G; Wong, G.F.; et al.; Natal molecular cloud of SNR Kes 41. Complete characterisation; EDP Sciences; Astronomy and Astrophysics; 619; 108; 11-2018; 1-7
0004-6361
CONICET Digital
CONICET
url http://hdl.handle.net/11336/97565
identifier_str_mv Supán, Jorge Leonardo; Castelletti, Gabriela Marta; Supanitsky, Alberto Daniel; Burton, M.G; Wong, G.F.; et al.; Natal molecular cloud of SNR Kes 41. Complete characterisation; EDP Sciences; Astronomy and Astrophysics; 619; 108; 11-2018; 1-7
0004-6361
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2018/11/aa33183-18/aa33183-18.html
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201833183
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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score 13.070432

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