Evidence of non-thermal x-ray emission from HH 80

Autores
Bonito, Rosaria; Lopez Santiago, Javier; Peri, Cintia Soledad; de Castro, Elisa; Benaglia, Paula; Albacete Colombo, Juan Facundo; Miceli, Marco
Año de publicación
2013
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separated, with the soft X-ray emission region situated behind the region of hard X-ray emission. We propose a scenario for HH 80 where soft X-ray emission is associated with thermal processes from the interaction of the jet with denser ambient matter and hard X-ray emission is produced by synchrotron radiation at the front shock.
Fil: Bonito, Rosaria. Istituto Nazionale Di Astrofisica; Italia
Fil: Lopez Santiago, Javier. Universidad Complutense de Madrid; España
Fil: Peri, Cintia Soledad. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: de Castro, Elisa. Universidad Complutense de Madrid; España
Fil: Benaglia, Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Albacete Colombo, Juan Facundo. Universidad Nacional del Comahue. Centro Universidad Región Zona Atlántica; Argentina
Fil: Miceli, Marco. Istituto Nazionale Di Astrofisica; Italia
Materia
HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIATION MECHANISMS: NON-THERMAL
STARS: INDIVIDUAL
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:11336/3269
Acceder
id CONICETDig_3302d068eb46fec001311306bad81604
oai_identifier_str oai:ri.conicet.gov.ar:11336/3269
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Evidence of non-thermal x-ray emission from HH 80Bonito, RosariaLopez Santiago, JavierPeri, Cintia Soledadde Castro, ElisaBenaglia, PaulaAlbacete Colombo, Juan FacundoMiceli, MarcoHERBIG-HARO OBJECTSISM: JETS AND OUTFLOWSRADIATION MECHANISMS: NON-THERMALSTARS: INDIVIDUALhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separated, with the soft X-ray emission region situated behind the region of hard X-ray emission. We propose a scenario for HH 80 where soft X-ray emission is associated with thermal processes from the interaction of the jet with denser ambient matter and hard X-ray emission is produced by synchrotron radiation at the front shock.Fil: Bonito, Rosaria. Istituto Nazionale Di Astrofisica; ItaliaFil: Lopez Santiago, Javier. Universidad Complutense de Madrid; EspañaFil: Peri, Cintia Soledad. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: de Castro, Elisa. Universidad Complutense de Madrid; EspañaFil: Benaglia, Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: Albacete Colombo, Juan Facundo. Universidad Nacional del Comahue. Centro Universidad Región Zona Atlántica; ArgentinaFil: Miceli, Marco. Istituto Nazionale Di Astrofisica; ItaliaIop Publishing2013-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/3269Bonito, Rosaria; Lopez Santiago, Javier; Peri, Cintia Soledad; de Castro, Elisa; Benaglia, Paula; et al.; Evidence of non-thermal x-ray emission from HH 80; Iop Publishing; Astrophysical Journal Letters; 776; 2; 10-2013; 22-260004-637X2041-8213enginfo:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/776/2/L22info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/2041-8205/776/2/L22info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1309.4256info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T12:04:09Zoai:ri.conicet.gov.ar:11336/3269instacron: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:34982025-10-22 12:04:09.465CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Evidence of non-thermal x-ray emission from HH 80
title Evidence of non-thermal x-ray emission from HH 80
spellingShingle Evidence of non-thermal x-ray emission from HH 80
Bonito, Rosaria
HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIATION MECHANISMS: NON-THERMAL
STARS: INDIVIDUAL
title_short Evidence of non-thermal x-ray emission from HH 80
title_full Evidence of non-thermal x-ray emission from HH 80
title_fullStr Evidence of non-thermal x-ray emission from HH 80
title_full_unstemmed Evidence of non-thermal x-ray emission from HH 80
title_sort Evidence of non-thermal x-ray emission from HH 80
dc.creator.none.fl_str_mv Bonito, Rosaria
Lopez Santiago, Javier
Peri, Cintia Soledad
de Castro, Elisa
Benaglia, Paula
Albacete Colombo, Juan Facundo
Miceli, Marco
author Bonito, Rosaria
author_facet Bonito, Rosaria
Lopez Santiago, Javier
Peri, Cintia Soledad
de Castro, Elisa
Benaglia, Paula
Albacete Colombo, Juan Facundo
Miceli, Marco
author_role author
author2 Lopez Santiago, Javier
Peri, Cintia Soledad
de Castro, Elisa
Benaglia, Paula
Albacete Colombo, Juan Facundo
Miceli, Marco
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIATION MECHANISMS: NON-THERMAL
STARS: INDIVIDUAL
topic HERBIG-HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIATION MECHANISMS: NON-THERMAL
STARS: INDIVIDUAL
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separated, with the soft X-ray emission region situated behind the region of hard X-ray emission. We propose a scenario for HH 80 where soft X-ray emission is associated with thermal processes from the interaction of the jet with denser ambient matter and hard X-ray emission is produced by synchrotron radiation at the front shock.
Fil: Bonito, Rosaria. Istituto Nazionale Di Astrofisica; Italia
Fil: Lopez Santiago, Javier. Universidad Complutense de Madrid; España
Fil: Peri, Cintia Soledad. Universidad Nacional de la Plata. Facultad de Ciencias Astronómicas y Geofísicas; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: de Castro, Elisa. Universidad Complutense de Madrid; España
Fil: Benaglia, Paula. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico La Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Albacete Colombo, Juan Facundo. Universidad Nacional del Comahue. Centro Universidad Región Zona Atlántica; Argentina
Fil: Miceli, Marco. Istituto Nazionale Di Astrofisica; Italia
description Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separated, with the soft X-ray emission region situated behind the region of hard X-ray emission. We propose a scenario for HH 80 where soft X-ray emission is associated with thermal processes from the interaction of the jet with denser ambient matter and hard X-ray emission is produced by synchrotron radiation at the front shock.
publishDate 2013
dc.date.none.fl_str_mv 2013-10
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/11336/3269
Bonito, Rosaria; Lopez Santiago, Javier; Peri, Cintia Soledad; de Castro, Elisa; Benaglia, Paula; et al.; Evidence of non-thermal x-ray emission from HH 80; Iop Publishing; Astrophysical Journal Letters; 776; 2; 10-2013; 22-26
0004-637X
2041-8213
url http://hdl.handle.net/11336/3269
identifier_str_mv Bonito, Rosaria; Lopez Santiago, Javier; Peri, Cintia Soledad; de Castro, Elisa; Benaglia, Paula; et al.; Evidence of non-thermal x-ray emission from HH 80; Iop Publishing; Astrophysical Journal Letters; 776; 2; 10-2013; 22-26
0004-637X
2041-8213
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/776/2/L22
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.1088/2041-8205/776/2/L22
info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1309.4256
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 Iop Publishing
publisher.none.fl_str_mv Iop Publishing
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
_version_ 1846782387959103488
score 12.982451

Publicaciones similares