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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/3269
Ver los metadatos del registro completo
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 Técnicas2025-09-29T10:31:43Zoai: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:34982025-09-29 10:31:43.85CONICET 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_ |
1844614328624349184 |
score |
13.070432 |