A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer

Autores
López García, M. A.; López Santiago, J.; Albacete Colombo, Juan Facundo; Pérez González, P. G.; De Castro, E.
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Fil: López García, M. A. Universidad Complutense de Madrid; España
Fil: López Santiago, J. Universidad Complutense de Madrid; España
Fil: Albacete Colombo, Juan F. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Albacete Colombo, Juan F. Universidad Nacional del Comahue. Centro Universidad Región Zona Atlántica; Argentina
Fil: Pérez González, P. G. . Universidad Complutense de Madrid; España
Fil: De Castro, E.. Universidad Complutense de Madrid; España
Nearby star-forming regions are ideal laboratories to study high-energy emission of different stellar populations, from very massive stars to brown dwarfs. NGC 2023 is a reflection nebula situated to the south of the Flame Nebula (NGC 2024) and at the edge of the H II region IC 434, which also contains the Horsehead Nebula (Barnard 33). NGC 2023, NGC 2024, Barnard 33 and the surroundings of the O-type supergiant star ζ Ori constitute the south part of the Orion B molecular complex. In this work, we present a comprehensive study of X-ray emitters in the region of NGC 2023 and its surroundings. We combine optical and infrared data to determine physical properties (mass, temperature, luminosity and the presence of accretion discs) of the stars detected in an XMM–Newton observation. This study has allowed us to analyse spectral energy distribution of these stars for the first time and determine their evolutionary stage. Properties of the X-ray emitting plasma of these stars are compared to those found in other nearby star-forming regions. The results indicate that the stars that are being formed in this region have characteristics, in terms of physical properties and luminosity function, similar to those found in the Taurus–Auriga molecular complex.
Materia
Astronomía
Stars: Coronae
Stars: Pre-Main-Sequence
Open Clusters and Associations: General
X-rays: Stars
Astronomía
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/4.0/
Repositorio
RID-UNRN (UNRN)
Institución
Universidad Nacional de Río Negro
OAI Identificador
oai:rid.unrn.edu.ar:20.500.12049/2498

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network_name_str RID-UNRN (UNRN)
spelling A comprehensive study of NGC 2023 withXMM–NewtonandSpitzerLópez García, M. A.López Santiago, J.Albacete Colombo, Juan FacundoPérez González, P. G.De Castro, E.AstronomíaStars: CoronaeStars: Pre-Main-SequenceOpen Clusters and Associations: GeneralX-rays: StarsAstronomíaFil: López García, M. A. Universidad Complutense de Madrid; EspañaFil: López Santiago, J. Universidad Complutense de Madrid; EspañaFil: Albacete Colombo, Juan F. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Albacete Colombo, Juan F. Universidad Nacional del Comahue. Centro Universidad Región Zona Atlántica; ArgentinaFil: Pérez González, P. G. . Universidad Complutense de Madrid; EspañaFil: De Castro, E.. Universidad Complutense de Madrid; EspañaNearby star-forming regions are ideal laboratories to study high-energy emission of different stellar populations, from very massive stars to brown dwarfs. NGC 2023 is a reflection nebula situated to the south of the Flame Nebula (NGC 2024) and at the edge of the H II region IC 434, which also contains the Horsehead Nebula (Barnard 33). NGC 2023, NGC 2024, Barnard 33 and the surroundings of the O-type supergiant star ζ Ori constitute the south part of the Orion B molecular complex. In this work, we present a comprehensive study of X-ray emitters in the region of NGC 2023 and its surroundings. We combine optical and infrared data to determine physical properties (mass, temperature, luminosity and the presence of accretion discs) of the stars detected in an XMM–Newton observation. This study has allowed us to analyse spectral energy distribution of these stars for the first time and determine their evolutionary stage. Properties of the X-ray emitting plasma of these stars are compared to those found in other nearby star-forming regions. The results indicate that the stars that are being formed in this region have characteristics, in terms of physical properties and luminosity function, similar to those found in the Taurus–Auriga molecular complex.2013-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfLópez García, M. A., López Santiago, J., Albacete Colombo, Juan F., Pérez González, P. G. & de Castro, E.(2013); A comprehensive study of NGC 2023 with XMM–Newton and Spitzer; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 429; 1; 1-2013; 775-7911365-29660035-8711http://dx.doi.org/10.1093/mnras/sts373http://mnras.oxfordjournals.org/content/429/1/775https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2498http://hdl.handle.net/11336/11040eng429Monthly Notices of the Royal Astronomical Societyinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/4.0/reponame:RID-UNRN (UNRN)instname:Universidad Nacional de Río Negro2025-09-29T14:29:09Zoai:rid.unrn.edu.ar:20.500.12049/2498instacron:UNRNInstitucionalhttps://rid.unrn.edu.ar/jspui/Universidad públicaNo correspondehttps://rid.unrn.edu.ar/oai/snrdrid@unrn.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:43692025-09-29 14:29:09.476RID-UNRN (UNRN) - Universidad Nacional de Río Negrofalse
dc.title.none.fl_str_mv A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
title A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
spellingShingle A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
López García, M. A.
Astronomía
Stars: Coronae
Stars: Pre-Main-Sequence
Open Clusters and Associations: General
X-rays: Stars
Astronomía
title_short A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
title_full A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
title_fullStr A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
title_full_unstemmed A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
title_sort A comprehensive study of NGC 2023 withXMM–NewtonandSpitzer
dc.creator.none.fl_str_mv López García, M. A.
López Santiago, J.
Albacete Colombo, Juan Facundo
Pérez González, P. G.
De Castro, E.
author López García, M. A.
author_facet López García, M. A.
López Santiago, J.
Albacete Colombo, Juan Facundo
Pérez González, P. G.
De Castro, E.
author_role author
author2 López Santiago, J.
Albacete Colombo, Juan Facundo
Pérez González, P. G.
De Castro, E.
author2_role author
author
author
author
dc.subject.none.fl_str_mv Astronomía
Stars: Coronae
Stars: Pre-Main-Sequence
Open Clusters and Associations: General
X-rays: Stars
Astronomía
topic Astronomía
Stars: Coronae
Stars: Pre-Main-Sequence
Open Clusters and Associations: General
X-rays: Stars
Astronomía
dc.description.none.fl_txt_mv Fil: López García, M. A. Universidad Complutense de Madrid; España
Fil: López Santiago, J. Universidad Complutense de Madrid; España
Fil: Albacete Colombo, Juan F. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Albacete Colombo, Juan F. Universidad Nacional del Comahue. Centro Universidad Región Zona Atlántica; Argentina
Fil: Pérez González, P. G. . Universidad Complutense de Madrid; España
Fil: De Castro, E.. Universidad Complutense de Madrid; España
Nearby star-forming regions are ideal laboratories to study high-energy emission of different stellar populations, from very massive stars to brown dwarfs. NGC 2023 is a reflection nebula situated to the south of the Flame Nebula (NGC 2024) and at the edge of the H II region IC 434, which also contains the Horsehead Nebula (Barnard 33). NGC 2023, NGC 2024, Barnard 33 and the surroundings of the O-type supergiant star ζ Ori constitute the south part of the Orion B molecular complex. In this work, we present a comprehensive study of X-ray emitters in the region of NGC 2023 and its surroundings. We combine optical and infrared data to determine physical properties (mass, temperature, luminosity and the presence of accretion discs) of the stars detected in an XMM–Newton observation. This study has allowed us to analyse spectral energy distribution of these stars for the first time and determine their evolutionary stage. Properties of the X-ray emitting plasma of these stars are compared to those found in other nearby star-forming regions. The results indicate that the stars that are being formed in this region have characteristics, in terms of physical properties and luminosity function, similar to those found in the Taurus–Auriga molecular complex.
description Fil: López García, M. A. Universidad Complutense de Madrid; España
publishDate 2013
dc.date.none.fl_str_mv 2013-01
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 López García, M. A., López Santiago, J., Albacete Colombo, Juan F., Pérez González, P. G. & de Castro, E.(2013); A comprehensive study of NGC 2023 with XMM–Newton and Spitzer; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 429; 1; 1-2013; 775-791
1365-2966
0035-8711
http://dx.doi.org/10.1093/mnras/sts373
http://mnras.oxfordjournals.org/content/429/1/775
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2498
http://hdl.handle.net/11336/11040
identifier_str_mv López García, M. A., López Santiago, J., Albacete Colombo, Juan F., Pérez González, P. G. & de Castro, E.(2013); A comprehensive study of NGC 2023 with XMM–Newton and Spitzer; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 429; 1; 1-2013; 775-791
1365-2966
0035-8711
url http://dx.doi.org/10.1093/mnras/sts373
http://mnras.oxfordjournals.org/content/429/1/775
https://rid.unrn.edu.ar/jspui/handle/20.500.12049/2498
http://hdl.handle.net/11336/11040
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 429
Monthly Notices of the Royal Astronomical Society
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/4.0/
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:RID-UNRN (UNRN)
instname:Universidad Nacional de Río Negro
reponame_str RID-UNRN (UNRN)
collection RID-UNRN (UNRN)
instname_str Universidad Nacional de Río Negro
repository.name.fl_str_mv RID-UNRN (UNRN) - Universidad Nacional de Río Negro
repository.mail.fl_str_mv rid@unrn.edu.ar
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