Radio emission from massive protostellar objects

Autores
Benaglia, Paula
Año de publicación
2011
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
The study of the formation of massive stars present complex challenges from both theoretical and observational points of view. The initial phases of evolution, for instance, remain almost hidden except at radio and IR wavelengths. In this article, after stating some of the problems of massive star formation, the role of radio observations to disclose the involved physics is discussed. Historical observational findings are briefly outlined, and the connection between low energy and high energy aspects of the phenomenon is addressed. Finally, data availability in the form of some new surveys is reported.
Fil: Benaglia, Paula. 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
XIII Latin American Regional IAU Meeting
Morelia
México
Universidad Autónoma de México
Materia
HII REGIONS
ISM: JETS, OUTFLOWS
PRE MAIN SEQUENCE STARS
STARS, MASS LOSS
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:11336/225116
Acceder
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oai_identifier_str oai:ri.conicet.gov.ar:11336/225116
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network_name_str CONICET Digital (CONICET)
spelling Radio emission from massive protostellar objectsBenaglia, PaulaHII REGIONSISM: JETS, OUTFLOWSPRE MAIN SEQUENCE STARSSTARS, MASS LOSShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The study of the formation of massive stars present complex challenges from both theoretical and observational points of view. The initial phases of evolution, for instance, remain almost hidden except at radio and IR wavelengths. In this article, after stating some of the problems of massive star formation, the role of radio observations to disclose the involved physics is discussed. Historical observational findings are briefly outlined, and the connection between low energy and high energy aspects of the phenomenon is addressed. Finally, data availability in the form of some new surveys is reported.Fil: Benaglia, Paula. 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; ArgentinaXIII Latin American Regional IAU MeetingMoreliaMéxicoUniversidad Autónoma de MéxicoUniversidad Autónoma de MéxicoHenney, W. J.Torres Peimbert, S.2011info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectConferenciaJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/225116Radio emission from massive protostellar objects; XIII Latin American Regional IAU Meeting; Morelia; México; 2010; 211-2161405-2059CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://www.astroscu.unam.mx/rmaa/RMxAC..40/PDF/RMxAC..40_pbenaglia.pdfinfo:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol40.htmlInternacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:53:36Zoai:ri.conicet.gov.ar:11336/225116instacron: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 09:53:36.684CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Radio emission from massive protostellar objects
title Radio emission from massive protostellar objects
spellingShingle Radio emission from massive protostellar objects
Benaglia, Paula
HII REGIONS
ISM: JETS, OUTFLOWS
PRE MAIN SEQUENCE STARS
STARS, MASS LOSS
title_short Radio emission from massive protostellar objects
title_full Radio emission from massive protostellar objects
title_fullStr Radio emission from massive protostellar objects
title_full_unstemmed Radio emission from massive protostellar objects
title_sort Radio emission from massive protostellar objects
dc.creator.none.fl_str_mv Benaglia, Paula
author Benaglia, Paula
author_facet Benaglia, Paula
author_role author
dc.contributor.none.fl_str_mv Henney, W. J.
Torres Peimbert, S.
dc.subject.none.fl_str_mv HII REGIONS
ISM: JETS, OUTFLOWS
PRE MAIN SEQUENCE STARS
STARS, MASS LOSS
topic HII REGIONS
ISM: JETS, OUTFLOWS
PRE MAIN SEQUENCE STARS
STARS, MASS LOSS
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv The study of the formation of massive stars present complex challenges from both theoretical and observational points of view. The initial phases of evolution, for instance, remain almost hidden except at radio and IR wavelengths. In this article, after stating some of the problems of massive star formation, the role of radio observations to disclose the involved physics is discussed. Historical observational findings are briefly outlined, and the connection between low energy and high energy aspects of the phenomenon is addressed. Finally, data availability in the form of some new surveys is reported.
Fil: Benaglia, Paula. 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
XIII Latin American Regional IAU Meeting
Morelia
México
Universidad Autónoma de México
description The study of the formation of massive stars present complex challenges from both theoretical and observational points of view. The initial phases of evolution, for instance, remain almost hidden except at radio and IR wavelengths. In this article, after stating some of the problems of massive star formation, the role of radio observations to disclose the involved physics is discussed. Historical observational findings are briefly outlined, and the connection between low energy and high energy aspects of the phenomenon is addressed. Finally, data availability in the form of some new surveys is reported.
publishDate 2011
dc.date.none.fl_str_mv 2011
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Conferencia
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/11336/225116
Radio emission from massive protostellar objects; XIII Latin American Regional IAU Meeting; Morelia; México; 2010; 211-216
1405-2059
CONICET Digital
CONICET
url http://hdl.handle.net/11336/225116
identifier_str_mv Radio emission from massive protostellar objects; XIII Latin American Regional IAU Meeting; Morelia; México; 2010; 211-216
1405-2059
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://www.astroscu.unam.mx/rmaa/RMxAC..40/PDF/RMxAC..40_pbenaglia.pdf
info:eu-repo/semantics/altIdentifier/url/https://www.astroscu.unam.mx/RMxAC/vol40.html
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.coverage.none.fl_str_mv Internacional
dc.publisher.none.fl_str_mv Universidad Autónoma de México
publisher.none.fl_str_mv Universidad Autónoma de México
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 13.070432

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