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
Institución: Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador: oai:ri.conicet.gov.ar:11336/268058

Acceder

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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 Técnicas2025-10-22T11:08:47Zoai: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:34982025-10-22 11:08:47.808CONICET 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) instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str	CONICET Digital (CONICET)
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repository.mail.fl_str_mv	dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters

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