The star forming region Monoceros R2 as a gamma-ray source
- Autores
- Martí, J.; Luque Escamilla, P. L.; Muñoz Arjonilla, A. J.; Sánchez Ayaso, E.; Munar Adrover, P.; Sánchez Sutil, J. R.; Romero, Gustavo Esteban; Paredes, J. M.; Combi, Jorge Ariel
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. After the release of the gamma-ray source catalog produced by the Fermi satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supernova remnants, etc.), theoretical expectations predict new classes of gamma-ray sources. In particular, gamma-ray emission could be associated with some of the early phases of stellar evolution, but this interesting possibility is still poorly understood.
Aims: The aim of this paper is to assess the possibility of the Fermi gamma-ray source 2FGL J0607.5-0618c being associated with the massive star forming region Monoceros R2.
Methods: A multi-wavelength analysis of the Monoceros R2 region is carried out using archival data at radio, infrared, X-ray, and gamma-ray wavelengths. The resulting observational properties are used to estimate the physical parameters needed to test the different physical scenarios.
Results: We confirm the 2FGL J0607.5-0618c detection with improved confidence over the Fermi two-year catalog. We find that a combined effect of the multiple young stellar objects in Monoceros R2 is a viable picture for the nature of the source.
Fil: Martí, J.. Universidad de Jaén; España
Fil: Luque Escamilla, P. L.. Universidad de Jaén; España
Fil: Muñoz Arjonilla, A. J.. Universidad de Jaén; España
Fil: Sánchez Ayaso, E.. Universidad de Jaén; España
Fil: Munar Adrover, P.. Universidad de Barcelona; España
Fil: Sánchez Sutil, J. R.. Universidad de Jaén; España
Fil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina
Fil: Paredes, J. M.. Universidad de Barcelona; España
Fil: Combi, Jorge Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina - Materia
-
Protostars
Massive stars
Flares
Radio continuum - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/4636
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The star forming region Monoceros R2 as a gamma-ray sourceMartí, J.Luque Escamilla, P. L.Muñoz Arjonilla, A. J.Sánchez Ayaso, E.Munar Adrover, P.Sánchez Sutil, J. R.Romero, Gustavo EstebanParedes, J. M.Combi, Jorge ArielProtostarsMassive starsFlaresRadio continuumhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Context. After the release of the gamma-ray source catalog produced by the Fermi satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supernova remnants, etc.), theoretical expectations predict new classes of gamma-ray sources. In particular, gamma-ray emission could be associated with some of the early phases of stellar evolution, but this interesting possibility is still poorly understood. <br /> Aims: The aim of this paper is to assess the possibility of the Fermi gamma-ray source 2FGL J0607.5-0618c being associated with the massive star forming region Monoceros R2. <br /> Methods: A multi-wavelength analysis of the Monoceros R2 region is carried out using archival data at radio, infrared, X-ray, and gamma-ray wavelengths. The resulting observational properties are used to estimate the physical parameters needed to test the different physical scenarios. <br /> Results: We confirm the 2FGL J0607.5-0618c detection with improved confidence over the Fermi two-year catalog. We find that a combined effect of the multiple young stellar objects in Monoceros R2 is a viable picture for the nature of the source.Fil: Martí, J.. Universidad de Jaén; EspañaFil: Luque Escamilla, P. L.. Universidad de Jaén; EspañaFil: Muñoz Arjonilla, A. J.. Universidad de Jaén; EspañaFil: Sánchez Ayaso, E.. Universidad de Jaén; EspañaFil: Munar Adrover, P.. Universidad de Barcelona; EspañaFil: Sánchez Sutil, J. R.. Universidad de Jaén; EspañaFil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaFil: Paredes, J. M.. Universidad de Barcelona; EspañaFil: Combi, Jorge Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; ArgentinaEDP Sciences2013-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/4636Martí, J.; Luque Escamilla, P. L.; Muñoz Arjonilla, A. J.; Sánchez Ayaso, E.; Munar Adrover, P.; et al.; The star forming region Monoceros R2 as a gamma-ray source; EDP Sciences; Astronomy and Astrophysics; 556; A131; 8-2013; 131-1390004-6361enginfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220791info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1307.1682info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2013/08/aa20791-12/aa20791-12.htmlinfo:eu-repo/semantics/altIdentifier/issn/0004-6361info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:54:37Zoai:ri.conicet.gov.ar:11336/4636instacron: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 09:54:37.298CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
The star forming region Monoceros R2 as a gamma-ray source |
title |
The star forming region Monoceros R2 as a gamma-ray source |
spellingShingle |
The star forming region Monoceros R2 as a gamma-ray source Martí, J. Protostars Massive stars Flares Radio continuum |
title_short |
The star forming region Monoceros R2 as a gamma-ray source |
title_full |
The star forming region Monoceros R2 as a gamma-ray source |
title_fullStr |
The star forming region Monoceros R2 as a gamma-ray source |
title_full_unstemmed |
The star forming region Monoceros R2 as a gamma-ray source |
title_sort |
The star forming region Monoceros R2 as a gamma-ray source |
dc.creator.none.fl_str_mv |
Martí, J. Luque Escamilla, P. L. Muñoz Arjonilla, A. J. Sánchez Ayaso, E. Munar Adrover, P. Sánchez Sutil, J. R. Romero, Gustavo Esteban Paredes, J. M. Combi, Jorge Ariel |
author |
Martí, J. |
author_facet |
Martí, J. Luque Escamilla, P. L. Muñoz Arjonilla, A. J. Sánchez Ayaso, E. Munar Adrover, P. Sánchez Sutil, J. R. Romero, Gustavo Esteban Paredes, J. M. Combi, Jorge Ariel |
author_role |
author |
author2 |
Luque Escamilla, P. L. Muñoz Arjonilla, A. J. Sánchez Ayaso, E. Munar Adrover, P. Sánchez Sutil, J. R. Romero, Gustavo Esteban Paredes, J. M. Combi, Jorge Ariel |
author2_role |
author author author author author author author author |
dc.subject.none.fl_str_mv |
Protostars Massive stars Flares Radio continuum |
topic |
Protostars Massive stars Flares Radio continuum |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
Context. After the release of the gamma-ray source catalog produced by the Fermi satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supernova remnants, etc.), theoretical expectations predict new classes of gamma-ray sources. In particular, gamma-ray emission could be associated with some of the early phases of stellar evolution, but this interesting possibility is still poorly understood. <br /> Aims: The aim of this paper is to assess the possibility of the Fermi gamma-ray source 2FGL J0607.5-0618c being associated with the massive star forming region Monoceros R2. <br /> Methods: A multi-wavelength analysis of the Monoceros R2 region is carried out using archival data at radio, infrared, X-ray, and gamma-ray wavelengths. The resulting observational properties are used to estimate the physical parameters needed to test the different physical scenarios. <br /> Results: We confirm the 2FGL J0607.5-0618c detection with improved confidence over the Fermi two-year catalog. We find that a combined effect of the multiple young stellar objects in Monoceros R2 is a viable picture for the nature of the source. Fil: Martí, J.. Universidad de Jaén; España Fil: Luque Escamilla, P. L.. Universidad de Jaén; España Fil: Muñoz Arjonilla, A. J.. Universidad de Jaén; España Fil: Sánchez Ayaso, E.. Universidad de Jaén; España Fil: Munar Adrover, P.. Universidad de Barcelona; España Fil: Sánchez Sutil, J. R.. Universidad de Jaén; España Fil: Romero, Gustavo Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina Fil: Paredes, J. M.. Universidad de Barcelona; España Fil: Combi, Jorge Ariel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina |
description |
Context. After the release of the gamma-ray source catalog produced by the Fermi satellite during its first two years of operation, a significant fraction of sources still remain unassociated at lower energies. In addition to well-known high-energy emitters (pulsars, blazars, supernova remnants, etc.), theoretical expectations predict new classes of gamma-ray sources. In particular, gamma-ray emission could be associated with some of the early phases of stellar evolution, but this interesting possibility is still poorly understood. <br /> Aims: The aim of this paper is to assess the possibility of the Fermi gamma-ray source 2FGL J0607.5-0618c being associated with the massive star forming region Monoceros R2. <br /> Methods: A multi-wavelength analysis of the Monoceros R2 region is carried out using archival data at radio, infrared, X-ray, and gamma-ray wavelengths. The resulting observational properties are used to estimate the physical parameters needed to test the different physical scenarios. <br /> Results: We confirm the 2FGL J0607.5-0618c detection with improved confidence over the Fermi two-year catalog. We find that a combined effect of the multiple young stellar objects in Monoceros R2 is a viable picture for the nature of the source. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-08 |
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/11336/4636 Martí, J.; Luque Escamilla, P. L.; Muñoz Arjonilla, A. J.; Sánchez Ayaso, E.; Munar Adrover, P.; et al.; The star forming region Monoceros R2 as a gamma-ray source; EDP Sciences; Astronomy and Astrophysics; 556; A131; 8-2013; 131-139 0004-6361 |
url |
http://hdl.handle.net/11336/4636 |
identifier_str_mv |
Martí, J.; Luque Escamilla, P. L.; Muñoz Arjonilla, A. J.; Sánchez Ayaso, E.; Munar Adrover, P.; et al.; The star forming region Monoceros R2 as a gamma-ray source; EDP Sciences; Astronomy and Astrophysics; 556; A131; 8-2013; 131-139 0004-6361 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220791 info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1307.1682 info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2013/08/aa20791-12/aa20791-12.html info:eu-repo/semantics/altIdentifier/issn/0004-6361 |
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/ |
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application/pdf application/pdf application/pdf application/pdf |
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EDP Sciences |
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EDP Sciences |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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