ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters

Autores
Towner, A. P. M.; Ginsburg, A.; Della Vedova, Juan Pablo; Gusdorf, A.; Bontemps, Sophie; Csengeri, T.; Galván Madrid, R.; Louvet, F. K.; Motte, F.; Sanhueza, P.; Stutz, A. M.; Bally, J.; Baug, T.; Chen, H. R. V.; Cunningham, N.; Fernandez Lopez, Manuel; Liu, H. L.; Lu, X.; Nony, T.; Valeille Manet, M.; Wu, B.; Álvarez Gutiérrez, R. H.; Bonfand, M.; Di Francesco, J.; Nguyen Luong, Q.; Olguin, F.; Whitworth, A. P.
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present a catalog of 315 protostellar outflow candidates detected in SiO J = 5 - 4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km s-1 velocity resolution, and 2-12 mJy beam-1 (0.18-0.8 K) sensitivity. We find median outflow masses, momenta, and kinetic energies of ~0.3 M ⊙, 4 M ⊙ km s-1, and 1045 erg, respectively. Median outflow lifetimes are 6000 yr, yielding median mass, momentum, and energy rates of M˙ = 10-4.4 M ⊙ yr-1, P˙ = 10-3.2 M ⊙ km s-1 yr-1, and E˙ = 1 L ⊙. We analyze these outflow properties in the aggregate in each field. We find correlations between field-aggregated SiO outflow properties and total mass in cores (~3σ-5σ), and no correlations above 3σ with clump mass, clump luminosity, or clump luminosity-to-mass ratio. We perform a linear regression analysis and find that the correlation between field-aggregated outflow mass and total clump mass-which has been previously described in the literature-may actually be mediated by the relationship between outflow mass and total mass in cores. We also find that the most massive SiO outflow in each field is typically responsible for only 15%-30% of the total outflow mass (60% upper limit). Our data agree well with the established mechanical force-bolometric luminosity relationship in the literature, and our data extend this relationship up to L ≥ 106 L ⊙ and P˙ ≥ 1 M ⊙ km s-1 yr-1. Our lack of correlation with clump L/M is inconsistent with models of protocluster formation in which all protostars start forming at the same time.
Fil: Towner, A. P. M.. University of Arizona; Estados Unidos
Fil: Ginsburg, A.. University of Florida; Estados Unidos
Fil: Della Vedova, Juan Pablo. Centre National de la Recherche Scientifique; Francia. Université PSL; Francia
Fil: Gusdorf, A.. Sorbonne Université; Francia
Fil: Bontemps, Sophie. Universite de Bordeaux; Francia
Fil: Csengeri, T.. Universite de Bordeaux; Francia
Fil: Galván Madrid, R.. Universidad Nacional Autónoma de México; México
Fil: Louvet, F. K.. Universite Grenoble Alpes; Francia
Fil: Motte, F.. Universite Grenoble Alpes; Francia
Fil: Sanhueza, P.. National Astronomical Observatory of Japan; Japón
Fil: Stutz, A. M.. Universidad de Concepción; Chile
Fil: Bally, J.. University of Colorado; Estados Unidos
Fil: Baug, T.. S.N. Bose National Centre for Basic Sciences; India
Fil: Chen, H. R. V.. National Tsing Hua University; China
Fil: Cunningham, N.. Universite Grenoble Alpes; Francia
Fil: Fernandez Lopez, Manuel. 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
Fil: Liu, H. L.. Yunnan University; China
Fil: Lu, X.. Chinese Academy of Sciences; República de China
Fil: Nony, T.. Universidad Nacional Autónoma de México; México
Fil: Valeille Manet, M.. Universite de Bordeaux; Francia
Fil: Wu, B.. National Astronomical Observatory of Japan; Japón
Fil: Álvarez Gutiérrez, R. H.. Universidad de Concepción; Chile
Fil: Bonfand, M.. University of Virginia; Estados Unidos
Fil: Di Francesco, J.. National Research Council Of Canada; Canadá
Fil: Nguyen Luong, Q.. The American University of Paris; Francia
Fil: Olguin, F.. National Tsing Hua University; China
Fil: Whitworth, A. P.. Cardiff University; Reino Unido
Materia
Protostars
Astrochemistry
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:11336/268058

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spelling ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive ProtoclustersTowner, A. P. M.Ginsburg, A.Della Vedova, Juan PabloGusdorf, A.Bontemps, SophieCsengeri, T.Galván Madrid, R.Louvet, F. K.Motte, F.Sanhueza, P.Stutz, A. M.Bally, J.Baug, T.Chen, H. R. V.Cunningham, N.Fernandez Lopez, ManuelLiu, H. L.Lu, X.Nony, T.Valeille Manet, M.Wu, B.Álvarez Gutiérrez, R. H.Bonfand, M.Di Francesco, J.Nguyen Luong, Q.Olguin, F.Whitworth, A. P.ProtostarsAstrochemistryhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a catalog of 315 protostellar outflow candidates detected in SiO J = 5 - 4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km s-1 velocity resolution, and 2-12 mJy beam-1 (0.18-0.8 K) sensitivity. We find median outflow masses, momenta, and kinetic energies of ~0.3 M ⊙, 4 M ⊙ km s-1, and 1045 erg, respectively. Median outflow lifetimes are 6000 yr, yielding median mass, momentum, and energy rates of M˙ = 10-4.4 M ⊙ yr-1, P˙ = 10-3.2 M ⊙ km s-1 yr-1, and E˙ = 1 L ⊙. We analyze these outflow properties in the aggregate in each field. We find correlations between field-aggregated SiO outflow properties and total mass in cores (~3σ-5σ), and no correlations above 3σ with clump mass, clump luminosity, or clump luminosity-to-mass ratio. We perform a linear regression analysis and find that the correlation between field-aggregated outflow mass and total clump mass-which has been previously described in the literature-may actually be mediated by the relationship between outflow mass and total mass in cores. We also find that the most massive SiO outflow in each field is typically responsible for only 15%-30% of the total outflow mass (60% upper limit). Our data agree well with the established mechanical force-bolometric luminosity relationship in the literature, and our data extend this relationship up to L ≥ 106 L ⊙ and P˙ ≥ 1 M ⊙ km s-1 yr-1. Our lack of correlation with clump L/M is inconsistent with models of protocluster formation in which all protostars start forming at the same time.Fil: Towner, A. P. M.. University of Arizona; Estados UnidosFil: Ginsburg, A.. University of Florida; Estados UnidosFil: Della Vedova, Juan Pablo. Centre National de la Recherche Scientifique; Francia. Université PSL; FranciaFil: Gusdorf, A.. Sorbonne Université; FranciaFil: Bontemps, Sophie. Universite de Bordeaux; FranciaFil: Csengeri, T.. Universite de Bordeaux; FranciaFil: Galván Madrid, R.. Universidad Nacional Autónoma de México; MéxicoFil: Louvet, F. K.. Universite Grenoble Alpes; FranciaFil: Motte, F.. Universite Grenoble Alpes; FranciaFil: Sanhueza, P.. National Astronomical Observatory of Japan; JapónFil: Stutz, A. M.. Universidad de Concepción; ChileFil: Bally, J.. University of Colorado; Estados UnidosFil: Baug, T.. S.N. Bose National Centre for Basic Sciences; IndiaFil: Chen, H. R. V.. National Tsing Hua University; ChinaFil: Cunningham, N.. Universite Grenoble Alpes; FranciaFil: Fernandez Lopez, Manuel. 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; ArgentinaFil: Liu, H. L.. Yunnan University; ChinaFil: Lu, X.. Chinese Academy of Sciences; República de ChinaFil: Nony, T.. Universidad Nacional Autónoma de México; MéxicoFil: Valeille Manet, M.. Universite de Bordeaux; FranciaFil: Wu, B.. National Astronomical Observatory of Japan; JapónFil: Álvarez Gutiérrez, R. H.. Universidad de Concepción; ChileFil: Bonfand, M.. University of Virginia; Estados UnidosFil: Di Francesco, J.. National Research Council Of Canada; CanadáFil: Nguyen Luong, Q.. The American University of Paris; FranciaFil: Olguin, F.. National Tsing Hua University; ChinaFil: Whitworth, A. P.. Cardiff University; Reino UnidoIOP Publishing2023-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/268058Towner, A. P. M.; Ginsburg, A.; Della Vedova, Juan Pablo; Gusdorf, A.; Bontemps, Sophie; et al.; ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters; IOP Publishing; Astrophysical Journal; 960; 1; 12-2023; 1-280004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad0786info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad0786info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:40:14Zoai:ri.conicet.gov.ar:11336/268058instacron: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 09:40:14.763CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
title ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
spellingShingle ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
Towner, A. P. M.
Protostars
Astrochemistry
title_short ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
title_full ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
title_fullStr ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
title_full_unstemmed ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
title_sort ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters
dc.creator.none.fl_str_mv Towner, A. P. M.
Ginsburg, A.
Della Vedova, Juan Pablo
Gusdorf, A.
Bontemps, Sophie
Csengeri, T.
Galván Madrid, R.
Louvet, F. K.
Motte, F.
Sanhueza, P.
Stutz, A. M.
Bally, J.
Baug, T.
Chen, H. R. V.
Cunningham, N.
Fernandez Lopez, Manuel
Liu, H. L.
Lu, X.
Nony, T.
Valeille Manet, M.
Wu, B.
Álvarez Gutiérrez, R. H.
Bonfand, M.
Di Francesco, J.
Nguyen Luong, Q.
Olguin, F.
Whitworth, A. P.
author Towner, A. P. M.
author_facet Towner, A. P. M.
Ginsburg, A.
Della Vedova, Juan Pablo
Gusdorf, A.
Bontemps, Sophie
Csengeri, T.
Galván Madrid, R.
Louvet, F. K.
Motte, F.
Sanhueza, P.
Stutz, A. M.
Bally, J.
Baug, T.
Chen, H. R. V.
Cunningham, N.
Fernandez Lopez, Manuel
Liu, H. L.
Lu, X.
Nony, T.
Valeille Manet, M.
Wu, B.
Álvarez Gutiérrez, R. H.
Bonfand, M.
Di Francesco, J.
Nguyen Luong, Q.
Olguin, F.
Whitworth, A. P.
author_role author
author2 Ginsburg, A.
Della Vedova, Juan Pablo
Gusdorf, A.
Bontemps, Sophie
Csengeri, T.
Galván Madrid, R.
Louvet, F. K.
Motte, F.
Sanhueza, P.
Stutz, A. M.
Bally, J.
Baug, T.
Chen, H. R. V.
Cunningham, N.
Fernandez Lopez, Manuel
Liu, H. L.
Lu, X.
Nony, T.
Valeille Manet, M.
Wu, B.
Álvarez Gutiérrez, R. H.
Bonfand, M.
Di Francesco, J.
Nguyen Luong, Q.
Olguin, F.
Whitworth, A. P.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Protostars
Astrochemistry
topic Protostars
Astrochemistry
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present a catalog of 315 protostellar outflow candidates detected in SiO J = 5 - 4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km s-1 velocity resolution, and 2-12 mJy beam-1 (0.18-0.8 K) sensitivity. We find median outflow masses, momenta, and kinetic energies of ~0.3 M ⊙, 4 M ⊙ km s-1, and 1045 erg, respectively. Median outflow lifetimes are 6000 yr, yielding median mass, momentum, and energy rates of M˙ = 10-4.4 M ⊙ yr-1, P˙ = 10-3.2 M ⊙ km s-1 yr-1, and E˙ = 1 L ⊙. We analyze these outflow properties in the aggregate in each field. We find correlations between field-aggregated SiO outflow properties and total mass in cores (~3σ-5σ), and no correlations above 3σ with clump mass, clump luminosity, or clump luminosity-to-mass ratio. We perform a linear regression analysis and find that the correlation between field-aggregated outflow mass and total clump mass-which has been previously described in the literature-may actually be mediated by the relationship between outflow mass and total mass in cores. We also find that the most massive SiO outflow in each field is typically responsible for only 15%-30% of the total outflow mass (60% upper limit). Our data agree well with the established mechanical force-bolometric luminosity relationship in the literature, and our data extend this relationship up to L ≥ 106 L ⊙ and P˙ ≥ 1 M ⊙ km s-1 yr-1. Our lack of correlation with clump L/M is inconsistent with models of protocluster formation in which all protostars start forming at the same time.
Fil: Towner, A. P. M.. University of Arizona; Estados Unidos
Fil: Ginsburg, A.. University of Florida; Estados Unidos
Fil: Della Vedova, Juan Pablo. Centre National de la Recherche Scientifique; Francia. Université PSL; Francia
Fil: Gusdorf, A.. Sorbonne Université; Francia
Fil: Bontemps, Sophie. Universite de Bordeaux; Francia
Fil: Csengeri, T.. Universite de Bordeaux; Francia
Fil: Galván Madrid, R.. Universidad Nacional Autónoma de México; México
Fil: Louvet, F. K.. Universite Grenoble Alpes; Francia
Fil: Motte, F.. Universite Grenoble Alpes; Francia
Fil: Sanhueza, P.. National Astronomical Observatory of Japan; Japón
Fil: Stutz, A. M.. Universidad de Concepción; Chile
Fil: Bally, J.. University of Colorado; Estados Unidos
Fil: Baug, T.. S.N. Bose National Centre for Basic Sciences; India
Fil: Chen, H. R. V.. National Tsing Hua University; China
Fil: Cunningham, N.. Universite Grenoble Alpes; Francia
Fil: Fernandez Lopez, Manuel. 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
Fil: Liu, H. L.. Yunnan University; China
Fil: Lu, X.. Chinese Academy of Sciences; República de China
Fil: Nony, T.. Universidad Nacional Autónoma de México; México
Fil: Valeille Manet, M.. Universite de Bordeaux; Francia
Fil: Wu, B.. National Astronomical Observatory of Japan; Japón
Fil: Álvarez Gutiérrez, R. H.. Universidad de Concepción; Chile
Fil: Bonfand, M.. University of Virginia; Estados Unidos
Fil: Di Francesco, J.. National Research Council Of Canada; Canadá
Fil: Nguyen Luong, Q.. The American University of Paris; Francia
Fil: Olguin, F.. National Tsing Hua University; China
Fil: Whitworth, A. P.. Cardiff University; Reino Unido
description We present a catalog of 315 protostellar outflow candidates detected in SiO J = 5 - 4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km s-1 velocity resolution, and 2-12 mJy beam-1 (0.18-0.8 K) sensitivity. We find median outflow masses, momenta, and kinetic energies of ~0.3 M ⊙, 4 M ⊙ km s-1, and 1045 erg, respectively. Median outflow lifetimes are 6000 yr, yielding median mass, momentum, and energy rates of M˙ = 10-4.4 M ⊙ yr-1, P˙ = 10-3.2 M ⊙ km s-1 yr-1, and E˙ = 1 L ⊙. We analyze these outflow properties in the aggregate in each field. We find correlations between field-aggregated SiO outflow properties and total mass in cores (~3σ-5σ), and no correlations above 3σ with clump mass, clump luminosity, or clump luminosity-to-mass ratio. We perform a linear regression analysis and find that the correlation between field-aggregated outflow mass and total clump mass-which has been previously described in the literature-may actually be mediated by the relationship between outflow mass and total mass in cores. We also find that the most massive SiO outflow in each field is typically responsible for only 15%-30% of the total outflow mass (60% upper limit). Our data agree well with the established mechanical force-bolometric luminosity relationship in the literature, and our data extend this relationship up to L ≥ 106 L ⊙ and P˙ ≥ 1 M ⊙ km s-1 yr-1. Our lack of correlation with clump L/M is inconsistent with models of protocluster formation in which all protostars start forming at the same time.
publishDate 2023
dc.date.none.fl_str_mv 2023-12
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/11336/268058
Towner, A. P. M.; Ginsburg, A.; Della Vedova, Juan Pablo; Gusdorf, A.; Bontemps, Sophie; et al.; ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters; IOP Publishing; Astrophysical Journal; 960; 1; 12-2023; 1-28
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/268058
identifier_str_mv Towner, A. P. M.; Ginsburg, A.; Della Vedova, Juan Pablo; Gusdorf, A.; Bontemps, Sophie; et al.; ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters; IOP Publishing; Astrophysical Journal; 960; 1; 12-2023; 1-28
0004-637X
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://iopscience.iop.org/article/10.3847/1538-4357/ad0786
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad0786
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)
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reponame_str CONICET Digital (CONICET)
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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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