Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)

Autores
Rodríguez Kamenetzky, Adriana Raquel; Carrasco-González, Carlos; Torrelles, J. M.; Vlemmings, W. H. T.; Rodríguez, L. F.; Surcis, G.; Gómez, J. F.; Cantó, J.; Goddi, C.; Kim, J. S.; Kim, S. -W.; Añez-López, N.; Curiel, S.; van Langevelde, H. J.
Año de publicación
2020
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
The massive star-forming region W75N (B) is thought to host a cluster of massive protostars (VLA 1, VLA 2, and VLA 3) undergoing different evolutionary stages. In this work, we present radio continuum data with the highest sensitivity and angular resolution obtained to date in this region, using the VLA-A and covering a wide range of frequencies (4–48 GHz), which allowed us to study the morphology and the nature of the emission of the different radio continuum sources. We also performed complementary studies with multi-epoch Very Large Array (VLA) data and Atacama Large Millimeter Array (ALMA) archive data at 1.3 mm wavelength. We find that VLA 1 is driving a thermal radio jet at scales of ≈0.1 arcsec (≈130 au), but also shows signs of an incipient hypercompact H II region at scales of ≲1 arcsec (≲1300 au). VLA 3 is also driving a thermal radio jet at scales of a few tenths of arcsec (few hundred of au). We conclude that this jet is shock exciting the radio continuum sources Bc and VLA 4 (obscured Herbig–Haro objects), which show proper motions moving outward from VLA 3 at velocities of ≈112–118 km s−1. We have also detected three new weak radio continuum sources, two of them associated with millimetre continuum cores observed with ALMA, suggesting that these two sources are also embedded young stellar objects in this massive star-forming region.
Fil: Rodríguez Kamenetzky, Adriana Raquel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Carrasco-González, Carlos. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
Fil: Torrelles, J. M.. Institut de Ciències de L'espai; España
Fil: Vlemmings, W. H. T.. Chalmers University of Technology; Suecia
Fil: Rodríguez, L. F.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
Fil: Surcis, G.. Osservatorio Astronomico di Cagliari; Italia
Fil: Gómez, J. F.. Instituto de Astrofísica de Andalucía; España
Fil: Cantó, J.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
Fil: Goddi, C.. Leiden University. ALLEGRO/Leiden Observatory; Países Bajos
Fil: Kim, J. S.. Korea Astronomy and Space Science Institute; Corea del Sur
Fil: Kim, S. -W.. Korea Astronomy and Space Science Institute; Corea del Sur
Fil: Añez-López, N.. Institut de Ciencies de L´espai ; Consejo Superior de Investigaciones Cientificas;
Fil: Curiel, S.. Institut de Ciencies de L´espai ; Consejo Superior de Investigaciones Cientificas;
Fil: van Langevelde, H. J.. Leiden University; Países Bajos
Materia
H II REGIONS
HERBIG–HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIO CONTINUUM: ISM
STARS: MASSIVE
STARS: PROTOSTARS
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:11336/141210
Acceder
id CONICETDig_851aa501f3dd189d520b119310940b5f
oai_identifier_str oai:ri.conicet.gov.ar:11336/141210
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)Rodríguez Kamenetzky, Adriana RaquelCarrasco-González, CarlosTorrelles, J. M.Vlemmings, W. H. T.Rodríguez, L. F.Surcis, G.Gómez, J. F.Cantó, J.Goddi, C.Kim, J. S.Kim, S. -W.Añez-López, N.Curiel, S.van Langevelde, H. J.H II REGIONSHERBIG–HARO OBJECTSISM: JETS AND OUTFLOWSRADIO CONTINUUM: ISMSTARS: MASSIVESTARS: PROTOSTARShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1The massive star-forming region W75N (B) is thought to host a cluster of massive protostars (VLA 1, VLA 2, and VLA 3) undergoing different evolutionary stages. In this work, we present radio continuum data with the highest sensitivity and angular resolution obtained to date in this region, using the VLA-A and covering a wide range of frequencies (4–48 GHz), which allowed us to study the morphology and the nature of the emission of the different radio continuum sources. We also performed complementary studies with multi-epoch Very Large Array (VLA) data and Atacama Large Millimeter Array (ALMA) archive data at 1.3 mm wavelength. We find that VLA 1 is driving a thermal radio jet at scales of ≈0.1 arcsec (≈130 au), but also shows signs of an incipient hypercompact H II region at scales of ≲1 arcsec (≲1300 au). VLA 3 is also driving a thermal radio jet at scales of a few tenths of arcsec (few hundred of au). We conclude that this jet is shock exciting the radio continuum sources Bc and VLA 4 (obscured Herbig–Haro objects), which show proper motions moving outward from VLA 3 at velocities of ≈112–118 km s−1. We have also detected three new weak radio continuum sources, two of them associated with millimetre continuum cores observed with ALMA, suggesting that these two sources are also embedded young stellar objects in this massive star-forming region.Fil: Rodríguez Kamenetzky, Adriana Raquel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; ArgentinaFil: Carrasco-González, Carlos. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Torrelles, J. M.. Institut de Ciències de L'espai; EspañaFil: Vlemmings, W. H. T.. Chalmers University of Technology; SueciaFil: Rodríguez, L. F.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Surcis, G.. Osservatorio Astronomico di Cagliari; ItaliaFil: Gómez, J. F.. Instituto de Astrofísica de Andalucía; EspañaFil: Cantó, J.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Goddi, C.. Leiden University. ALLEGRO/Leiden Observatory; Países BajosFil: Kim, J. S.. Korea Astronomy and Space Science Institute; Corea del SurFil: Kim, S. -W.. Korea Astronomy and Space Science Institute; Corea del SurFil: Añez-López, N.. Institut de Ciencies de L´espai ; Consejo Superior de Investigaciones Cientificas;Fil: Curiel, S.. Institut de Ciencies de L´espai ; Consejo Superior de Investigaciones Cientificas;Fil: van Langevelde, H. J.. Leiden University; Países BajosWiley Blackwell Publishing, Inc2020-06info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/141210Rodríguez Kamenetzky, Adriana Raquel; Carrasco-González, Carlos; Torrelles, J. M.; Vlemmings, W. H. T.; Rodríguez, L. F.; et al.; Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B); Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 496; 3; 6-2020; 3128-31410035-87111365-2966CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staa1742/5860292info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/staa1742info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:31:29Zoai:ri.conicet.gov.ar:11336/141210instacron: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 10:31:29.53CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
title Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
spellingShingle Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
Rodríguez Kamenetzky, Adriana Raquel
H II REGIONS
HERBIG–HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIO CONTINUUM: ISM
STARS: MASSIVE
STARS: PROTOSTARS
title_short Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
title_full Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
title_fullStr Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
title_full_unstemmed Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
title_sort Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B)
dc.creator.none.fl_str_mv Rodríguez Kamenetzky, Adriana Raquel
Carrasco-González, Carlos
Torrelles, J. M.
Vlemmings, W. H. T.
Rodríguez, L. F.
Surcis, G.
Gómez, J. F.
Cantó, J.
Goddi, C.
Kim, J. S.
Kim, S. -W.
Añez-López, N.
Curiel, S.
van Langevelde, H. J.
author Rodríguez Kamenetzky, Adriana Raquel
author_facet Rodríguez Kamenetzky, Adriana Raquel
Carrasco-González, Carlos
Torrelles, J. M.
Vlemmings, W. H. T.
Rodríguez, L. F.
Surcis, G.
Gómez, J. F.
Cantó, J.
Goddi, C.
Kim, J. S.
Kim, S. -W.
Añez-López, N.
Curiel, S.
van Langevelde, H. J.
author_role author
author2 Carrasco-González, Carlos
Torrelles, J. M.
Vlemmings, W. H. T.
Rodríguez, L. F.
Surcis, G.
Gómez, J. F.
Cantó, J.
Goddi, C.
Kim, J. S.
Kim, S. -W.
Añez-López, N.
Curiel, S.
van Langevelde, H. J.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv H II REGIONS
HERBIG–HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIO CONTINUUM: ISM
STARS: MASSIVE
STARS: PROTOSTARS
topic H II REGIONS
HERBIG–HARO OBJECTS
ISM: JETS AND OUTFLOWS
RADIO CONTINUUM: ISM
STARS: MASSIVE
STARS: PROTOSTARS
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 massive star-forming region W75N (B) is thought to host a cluster of massive protostars (VLA 1, VLA 2, and VLA 3) undergoing different evolutionary stages. In this work, we present radio continuum data with the highest sensitivity and angular resolution obtained to date in this region, using the VLA-A and covering a wide range of frequencies (4–48 GHz), which allowed us to study the morphology and the nature of the emission of the different radio continuum sources. We also performed complementary studies with multi-epoch Very Large Array (VLA) data and Atacama Large Millimeter Array (ALMA) archive data at 1.3 mm wavelength. We find that VLA 1 is driving a thermal radio jet at scales of ≈0.1 arcsec (≈130 au), but also shows signs of an incipient hypercompact H II region at scales of ≲1 arcsec (≲1300 au). VLA 3 is also driving a thermal radio jet at scales of a few tenths of arcsec (few hundred of au). We conclude that this jet is shock exciting the radio continuum sources Bc and VLA 4 (obscured Herbig–Haro objects), which show proper motions moving outward from VLA 3 at velocities of ≈112–118 km s−1. We have also detected three new weak radio continuum sources, two of them associated with millimetre continuum cores observed with ALMA, suggesting that these two sources are also embedded young stellar objects in this massive star-forming region.
Fil: Rodríguez Kamenetzky, Adriana Raquel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Córdoba. Instituto de Astronomía Teórica y Experimental. Universidad Nacional de Córdoba. Observatorio Astronómico de Córdoba. Instituto de Astronomía Teórica y Experimental; Argentina
Fil: Carrasco-González, Carlos. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
Fil: Torrelles, J. M.. Institut de Ciències de L'espai; España
Fil: Vlemmings, W. H. T.. Chalmers University of Technology; Suecia
Fil: Rodríguez, L. F.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
Fil: Surcis, G.. Osservatorio Astronomico di Cagliari; Italia
Fil: Gómez, J. F.. Instituto de Astrofísica de Andalucía; España
Fil: Cantó, J.. Universidad Autónoma de México. Instituto de Radioastronomía y Astrofísica; México
Fil: Goddi, C.. Leiden University. ALLEGRO/Leiden Observatory; Países Bajos
Fil: Kim, J. S.. Korea Astronomy and Space Science Institute; Corea del Sur
Fil: Kim, S. -W.. Korea Astronomy and Space Science Institute; Corea del Sur
Fil: Añez-López, N.. Institut de Ciencies de L´espai ; Consejo Superior de Investigaciones Cientificas;
Fil: Curiel, S.. Institut de Ciencies de L´espai ; Consejo Superior de Investigaciones Cientificas;
Fil: van Langevelde, H. J.. Leiden University; Países Bajos
description The massive star-forming region W75N (B) is thought to host a cluster of massive protostars (VLA 1, VLA 2, and VLA 3) undergoing different evolutionary stages. In this work, we present radio continuum data with the highest sensitivity and angular resolution obtained to date in this region, using the VLA-A and covering a wide range of frequencies (4–48 GHz), which allowed us to study the morphology and the nature of the emission of the different radio continuum sources. We also performed complementary studies with multi-epoch Very Large Array (VLA) data and Atacama Large Millimeter Array (ALMA) archive data at 1.3 mm wavelength. We find that VLA 1 is driving a thermal radio jet at scales of ≈0.1 arcsec (≈130 au), but also shows signs of an incipient hypercompact H II region at scales of ≲1 arcsec (≲1300 au). VLA 3 is also driving a thermal radio jet at scales of a few tenths of arcsec (few hundred of au). We conclude that this jet is shock exciting the radio continuum sources Bc and VLA 4 (obscured Herbig–Haro objects), which show proper motions moving outward from VLA 3 at velocities of ≈112–118 km s−1. We have also detected three new weak radio continuum sources, two of them associated with millimetre continuum cores observed with ALMA, suggesting that these two sources are also embedded young stellar objects in this massive star-forming region.
publishDate 2020
dc.date.none.fl_str_mv 2020-06
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/11336/141210
Rodríguez Kamenetzky, Adriana Raquel; Carrasco-González, Carlos; Torrelles, J. M.; Vlemmings, W. H. T.; Rodríguez, L. F.; et al.; Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B); Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 496; 3; 6-2020; 3128-3141
0035-8711
1365-2966
CONICET Digital
CONICET
url http://hdl.handle.net/11336/141210
identifier_str_mv Rodríguez Kamenetzky, Adriana Raquel; Carrasco-González, Carlos; Torrelles, J. M.; Vlemmings, W. H. T.; Rodríguez, L. F.; et al.; Characterizing the radio continuum nature of sources in the massive star-forming region W75N (B); Wiley Blackwell Publishing, Inc; Monthly Notices of the Royal Astronomical Society; 496; 3; 6-2020; 3128-3141
0035-8711
1365-2966
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/staa1742/5860292
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/staa1742
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 Wiley Blackwell Publishing, Inc
publisher.none.fl_str_mv Wiley Blackwell Publishing, Inc
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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