Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048

Autores
Araudo, Anabella Teresa; Rodríguez, Luis Felipe
Año de publicación
2012
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Protostellar jets are present in the later stages of the stellarformation. Non-thermal radio emission has been detected from the jetsand hot spots of some massive protostars, indicating the presence ofrelativistic electrons there. We are interested in exploring if thesenon-thermal particles can emit also at γ-rays. In the presentcontribution we model the non-thermal emission produced in the jetsassociated with the massive protostar IRAS 18162-2048. We obtain thatthe γ-ray emission produced in this source is detectable by thecurrent facilities in the GeV domain.
Fil: Araudo, Anabella Teresa. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional Autónoma de México; México
Fil: Rodríguez, Luis Felipe. Universidad Nacional Autónoma de México; México
High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy
Heidelberg
Alemania
Max-Planck-Institut für Kernphysik
Materia
RADIATIVE PROCESSES: NON THERMAL
STARS: INDIVIDUAL: l: IRAS 18162-2048
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:11336/152862
Acceder
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spelling Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048Araudo, Anabella TeresaRodríguez, Luis FelipeRADIATIVE PROCESSES: NON THERMALSTARS: INDIVIDUAL: l: IRAS 18162-2048https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Protostellar jets are present in the later stages of the stellarformation. Non-thermal radio emission has been detected from the jetsand hot spots of some massive protostars, indicating the presence ofrelativistic electrons there. We are interested in exploring if thesenon-thermal particles can emit also at γ-rays. In the presentcontribution we model the non-thermal emission produced in the jetsassociated with the massive protostar IRAS 18162-2048. We obtain thatthe γ-ray emission produced in this source is detectable by thecurrent facilities in the GeV domain.Fil: Araudo, Anabella Teresa. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional Autónoma de México; MéxicoFil: Rodríguez, Luis Felipe. Universidad Nacional Autónoma de México; MéxicoHigh Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray AstronomyHeidelbergAlemaniaMax-Planck-Institut für KernphysikAmerican Institute of PhysicsAharonian, Felix A.Hofmann, WernerRieger, Frank M.2012info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/152862Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 281-28497807354112341551-7616CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4772252info:eu-repo/semantics/altIdentifier/doi/10.1063/1.4772252info:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4772252info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1210.3078v1Internacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-22T11:17:00Zoai:ri.conicet.gov.ar:11336/152862instacron: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 11:17:01.289CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
title Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
spellingShingle Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
Araudo, Anabella Teresa
RADIATIVE PROCESSES: NON THERMAL
STARS: INDIVIDUAL: l: IRAS 18162-2048
title_short Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
title_full Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
title_fullStr Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
title_full_unstemmed Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
title_sort Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048
dc.creator.none.fl_str_mv Araudo, Anabella Teresa
Rodríguez, Luis Felipe
author Araudo, Anabella Teresa
author_facet Araudo, Anabella Teresa
Rodríguez, Luis Felipe
author_role author
author2 Rodríguez, Luis Felipe
author2_role author
dc.contributor.none.fl_str_mv Aharonian, Felix A.
Hofmann, Werner
Rieger, Frank M.
dc.subject.none.fl_str_mv RADIATIVE PROCESSES: NON THERMAL
STARS: INDIVIDUAL: l: IRAS 18162-2048
topic RADIATIVE PROCESSES: NON THERMAL
STARS: INDIVIDUAL: l: IRAS 18162-2048
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 are present in the later stages of the stellarformation. Non-thermal radio emission has been detected from the jetsand hot spots of some massive protostars, indicating the presence ofrelativistic electrons there. We are interested in exploring if thesenon-thermal particles can emit also at γ-rays. In the presentcontribution we model the non-thermal emission produced in the jetsassociated with the massive protostar IRAS 18162-2048. We obtain thatthe γ-ray emission produced in this source is detectable by thecurrent facilities in the GeV domain.
Fil: Araudo, Anabella Teresa. Provincia de Buenos Aires. Gobernación. Comisión de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomía; Argentina. Universidad Nacional Autónoma de México; México
Fil: Rodríguez, Luis Felipe. Universidad Nacional Autónoma de México; México
High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy
Heidelberg
Alemania
Max-Planck-Institut für Kernphysik
description Protostellar jets are present in the later stages of the stellarformation. Non-thermal radio emission has been detected from the jetsand hot spots of some massive protostars, indicating the presence ofrelativistic electrons there. We are interested in exploring if thesenon-thermal particles can emit also at γ-rays. In the presentcontribution we model the non-thermal emission produced in the jetsassociated with the massive protostar IRAS 18162-2048. We obtain thatthe γ-ray emission produced in this source is detectable by thecurrent facilities in the GeV domain.
publishDate 2012
dc.date.none.fl_str_mv 2012
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Congreso
Journal
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/152862
Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 281-284
9780735411234
1551-7616
CONICET Digital
CONICET
url http://hdl.handle.net/11336/152862
identifier_str_mv Jets from massive protostars as gamma-ray sources: the case of IRAS 18162-2048; High Energy Gamma-Ray Astronomy: 5th International Meeting on High Energy Gamma-Ray Astronomy; Heidelberg; Alemania; 2012; 281-284
9780735411234
1551-7616
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4772252
info:eu-repo/semantics/altIdentifier/doi/10.1063/1.4772252
info:eu-repo/semantics/altIdentifier/url/https://aip.scitation.org/doi/10.1063/1.4772252
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1210.3078v1
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
application/pdf
dc.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv American Institute of Physics
publisher.none.fl_str_mv American Institute of Physics
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 12.982451

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