ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2)
- Autores
- Cunningham, N.; Ginsburg, A.; Galván Madrid, R.; Motte, F.; Csengeri, T.; Stutz, A. M.; Fernandez Lopez, Manuel; Álvarez Gutiérrez, R. H.; Armante, M.; Baug, T.; Bonfand, M.; Bontemps, Sophie; Braine, J.; Brouillet, N.; Busquets, Gabriel; Díaz González, D. J.; Di Francesco, J.; Gusdorf, A.; Herpin, F.; Liu, H.; López-Sepulcre, A.; Louvet, F.; Lu, X.; Maud, L.; Nony, T.; Olguin, F. A.; Pouteau, Y.; Rivera Soto, R.; Sandoval Garrido, N. A.; Sanhueza, P.; Tatematsu, K.; Towner, A. P. M.; Valeille Manet, M.
- Año de publicación
- 2023
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their early evolutionary stages. It further aims to understand their kinematics, chemistry, and the impact of gas inflow, accretion, and dynamics on the CMF. We present here the first release of the ALMA-IMF line data cubes (DR1), produced from the combination of two ALMA 12 m-array configurations. The data include 12 spectral windows, with eight at 1.3 mm and four at 3 mm. The broad spectral coverage of ALMA-IMF (∼6.7 GHz bandwidth coverage per field) hosts a wealth of simple atomic, molecular, ionised, and complex organic molecular lines. We describe the line cube calibration done by ALMA and the subsequent calibration and imaging we performed. We discuss our choice of calibration parameters and optimisation of the cleaning parameters, and we demonstrate the utility and necessity of additional processing compared to the ALMA archive pipeline. As a demonstration of the scientific potential of these data, we present a first analysis of the DCN (3-2) line. We find that DCN (3-2) traces a diversity of morphologies and complex velocity structures, which tend to be more filamentary and widespread in evolved regions and are more compact in the young and intermediate-stage protoclusters. Furthermore, we used the DCN (3-2) emission as a tracer of the gas associated with 595 continuum cores across the 15 protoclusters, providing the first estimates of the core systemic velocities and linewidths within the sample. We find that DCN (3-2) is detected towards a higher percentage of cores in evolved regions than the young and intermediate-stage protoclusters and is likely a more complete tracer of the core population in more evolved protoclusters. The full ALMA 12m-array cubes for the ALMA-IMF Large Program are provided with this DR1 release.
Fil: Cunningham, N.. Universite Grenoble Alpes; Francia
Fil: Ginsburg, A.. University of Florida; Estados Unidos
Fil: Galván Madrid, R.. No especifíca;
Fil: Motte, F.. Universite Grenoble Alpes; Francia
Fil: Csengeri, T.. Universite de Bordeaux; Francia
Fil: Stutz, A. M.. Universidad de Concepción; Chile
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: Álvarez Gutiérrez, R. H.. Universidad de Concepción; Chile
Fil: Armante, M.. Universite de Bordeaux; Francia
Fil: Baug, T.. Bose National Centre For Basic Sciences; India
Fil: Bonfand, M.. Ecole Normale Supérieure; Francia
Fil: Bontemps, Sophie. Universite de Bordeaux; Francia
Fil: Braine, J.. Universite de Bordeaux; Francia
Fil: Brouillet, N.. Universite de Bordeaux; Francia
Fil: Busquets, Gabriel. Universidad de Barcelona; España
Fil: Díaz González, D. J.. Instituto de Radioastronomía y Astrofísica; México
Fil: Di Francesco, J.. National Research Council Of Canada; Canadá
Fil: Gusdorf, A.. Universite de Bordeaux; Francia
Fil: Herpin, F.. Ecole Normale Supérieure; Francia
Fil: Liu, H.. Yunnan University; China
Fil: López-Sepulcre, A.. Universite Grenoble Alpes; Francia
Fil: Louvet, F.. Universite Grenoble Alpes; Francia
Fil: Lu, X.. Chinese Academy of Sciences; República de China
Fil: Maud, L.. European Southern Observatory; Alemania
Fil: Nony, T.. Instituto de Radioastronomía y Astrofísica; México
Fil: Olguin, F. A.. National Tsing Hua University; China
Fil: Pouteau, Y.. Universite Grenoble Alpes; Francia
Fil: Rivera Soto, R.. Instituto de Radioastronomía y Astrofísica; México
Fil: Sandoval Garrido, N. A.. Universidad de Concepción; Chile
Fil: Sanhueza, P.. National Astronomical Observatory Of Japan; Japón
Fil: Tatematsu, K.. National Astronomical Observatory Of Japan; Japón
Fil: Towner, A. P. M.. University of Florida; Estados Unidos
Fil: Valeille Manet, M.. Universite de Bordeaux; Francia - Materia
-
instrumentation: interferometers
stars: formation
stars: massive
stars: kinematics and dynamics - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/251916
Ver los metadatos del registro completo
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ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2)Cunningham, N.Ginsburg, A.Galván Madrid, R.Motte, F.Csengeri, T.Stutz, A. M.Fernandez Lopez, ManuelÁlvarez Gutiérrez, R. H.Armante, M.Baug, T.Bonfand, M.Bontemps, SophieBraine, J.Brouillet, N.Busquets, GabrielDíaz González, D. J.Di Francesco, J.Gusdorf, A.Herpin, F.Liu, H.López-Sepulcre, A.Louvet, F.Lu, X.Maud, L.Nony, T.Olguin, F. A.Pouteau, Y.Rivera Soto, R.Sandoval Garrido, N. A.Sanhueza, P.Tatematsu, K.Towner, A. P. M.Valeille Manet, M.instrumentation: interferometersstars: formationstars: massivestars: kinematics and dynamicshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their early evolutionary stages. It further aims to understand their kinematics, chemistry, and the impact of gas inflow, accretion, and dynamics on the CMF. We present here the first release of the ALMA-IMF line data cubes (DR1), produced from the combination of two ALMA 12 m-array configurations. The data include 12 spectral windows, with eight at 1.3 mm and four at 3 mm. The broad spectral coverage of ALMA-IMF (∼6.7 GHz bandwidth coverage per field) hosts a wealth of simple atomic, molecular, ionised, and complex organic molecular lines. We describe the line cube calibration done by ALMA and the subsequent calibration and imaging we performed. We discuss our choice of calibration parameters and optimisation of the cleaning parameters, and we demonstrate the utility and necessity of additional processing compared to the ALMA archive pipeline. As a demonstration of the scientific potential of these data, we present a first analysis of the DCN (3-2) line. We find that DCN (3-2) traces a diversity of morphologies and complex velocity structures, which tend to be more filamentary and widespread in evolved regions and are more compact in the young and intermediate-stage protoclusters. Furthermore, we used the DCN (3-2) emission as a tracer of the gas associated with 595 continuum cores across the 15 protoclusters, providing the first estimates of the core systemic velocities and linewidths within the sample. We find that DCN (3-2) is detected towards a higher percentage of cores in evolved regions than the young and intermediate-stage protoclusters and is likely a more complete tracer of the core population in more evolved protoclusters. The full ALMA 12m-array cubes for the ALMA-IMF Large Program are provided with this DR1 release.Fil: Cunningham, N.. Universite Grenoble Alpes; FranciaFil: Ginsburg, A.. University of Florida; Estados UnidosFil: Galván Madrid, R.. No especifíca;Fil: Motte, F.. Universite Grenoble Alpes; FranciaFil: Csengeri, T.. Universite de Bordeaux; FranciaFil: Stutz, A. M.. Universidad de Concepción; ChileFil: 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: Álvarez Gutiérrez, R. H.. Universidad de Concepción; ChileFil: Armante, M.. Universite de Bordeaux; FranciaFil: Baug, T.. Bose National Centre For Basic Sciences; IndiaFil: Bonfand, M.. Ecole Normale Supérieure; FranciaFil: Bontemps, Sophie. Universite de Bordeaux; FranciaFil: Braine, J.. Universite de Bordeaux; FranciaFil: Brouillet, N.. Universite de Bordeaux; FranciaFil: Busquets, Gabriel. Universidad de Barcelona; EspañaFil: Díaz González, D. J.. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Di Francesco, J.. National Research Council Of Canada; CanadáFil: Gusdorf, A.. Universite de Bordeaux; FranciaFil: Herpin, F.. Ecole Normale Supérieure; FranciaFil: Liu, H.. Yunnan University; ChinaFil: López-Sepulcre, A.. Universite Grenoble Alpes; FranciaFil: Louvet, F.. Universite Grenoble Alpes; FranciaFil: Lu, X.. Chinese Academy of Sciences; República de ChinaFil: Maud, L.. European Southern Observatory; AlemaniaFil: Nony, T.. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Olguin, F. A.. National Tsing Hua University; ChinaFil: Pouteau, Y.. Universite Grenoble Alpes; FranciaFil: Rivera Soto, R.. Instituto de Radioastronomía y Astrofísica; MéxicoFil: Sandoval Garrido, N. A.. Universidad de Concepción; ChileFil: Sanhueza, P.. National Astronomical Observatory Of Japan; JapónFil: Tatematsu, K.. National Astronomical Observatory Of Japan; JapónFil: Towner, A. P. M.. University of Florida; Estados UnidosFil: Valeille Manet, M.. Universite de Bordeaux; FranciaEDP Sciences2023-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/251916Cunningham, N.; Ginsburg, A.; Galván Madrid, R.; Motte, F.; Csengeri, T.; et al.; ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2); EDP Sciences; Astronomy and Astrophysics; 678; 10-2023; 1-730004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/10.1051/0004-6361/202245429info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/202245429info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:06:53Zoai:ri.conicet.gov.ar:11336/251916instacron: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 10:06:53.967CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| title |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| spellingShingle |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) Cunningham, N. instrumentation: interferometers stars: formation stars: massive stars: kinematics and dynamics |
| title_short |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| title_full |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| title_fullStr |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| title_full_unstemmed |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| title_sort |
ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2) |
| dc.creator.none.fl_str_mv |
Cunningham, N. Ginsburg, A. Galván Madrid, R. Motte, F. Csengeri, T. Stutz, A. M. Fernandez Lopez, Manuel Álvarez Gutiérrez, R. H. Armante, M. Baug, T. Bonfand, M. Bontemps, Sophie Braine, J. Brouillet, N. Busquets, Gabriel Díaz González, D. J. Di Francesco, J. Gusdorf, A. Herpin, F. Liu, H. López-Sepulcre, A. Louvet, F. Lu, X. Maud, L. Nony, T. Olguin, F. A. Pouteau, Y. Rivera Soto, R. Sandoval Garrido, N. A. Sanhueza, P. Tatematsu, K. Towner, A. P. M. Valeille Manet, M. |
| author |
Cunningham, N. |
| author_facet |
Cunningham, N. Ginsburg, A. Galván Madrid, R. Motte, F. Csengeri, T. Stutz, A. M. Fernandez Lopez, Manuel Álvarez Gutiérrez, R. H. Armante, M. Baug, T. Bonfand, M. Bontemps, Sophie Braine, J. Brouillet, N. Busquets, Gabriel Díaz González, D. J. Di Francesco, J. Gusdorf, A. Herpin, F. Liu, H. López-Sepulcre, A. Louvet, F. Lu, X. Maud, L. Nony, T. Olguin, F. A. Pouteau, Y. Rivera Soto, R. Sandoval Garrido, N. A. Sanhueza, P. Tatematsu, K. Towner, A. P. M. Valeille Manet, M. |
| author_role |
author |
| author2 |
Ginsburg, A. Galván Madrid, R. Motte, F. Csengeri, T. Stutz, A. M. Fernandez Lopez, Manuel Álvarez Gutiérrez, R. H. Armante, M. Baug, T. Bonfand, M. Bontemps, Sophie Braine, J. Brouillet, N. Busquets, Gabriel Díaz González, D. J. Di Francesco, J. Gusdorf, A. Herpin, F. Liu, H. López-Sepulcre, A. Louvet, F. Lu, X. Maud, L. Nony, T. Olguin, F. A. Pouteau, Y. Rivera Soto, R. Sandoval Garrido, N. A. Sanhueza, P. Tatematsu, K. Towner, A. P. M. Valeille Manet, M. |
| 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 author author author author author author |
| dc.subject.none.fl_str_mv |
instrumentation: interferometers stars: formation stars: massive stars: kinematics and dynamics |
| topic |
instrumentation: interferometers stars: formation stars: massive stars: kinematics and dynamics |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their early evolutionary stages. It further aims to understand their kinematics, chemistry, and the impact of gas inflow, accretion, and dynamics on the CMF. We present here the first release of the ALMA-IMF line data cubes (DR1), produced from the combination of two ALMA 12 m-array configurations. The data include 12 spectral windows, with eight at 1.3 mm and four at 3 mm. The broad spectral coverage of ALMA-IMF (∼6.7 GHz bandwidth coverage per field) hosts a wealth of simple atomic, molecular, ionised, and complex organic molecular lines. We describe the line cube calibration done by ALMA and the subsequent calibration and imaging we performed. We discuss our choice of calibration parameters and optimisation of the cleaning parameters, and we demonstrate the utility and necessity of additional processing compared to the ALMA archive pipeline. As a demonstration of the scientific potential of these data, we present a first analysis of the DCN (3-2) line. We find that DCN (3-2) traces a diversity of morphologies and complex velocity structures, which tend to be more filamentary and widespread in evolved regions and are more compact in the young and intermediate-stage protoclusters. Furthermore, we used the DCN (3-2) emission as a tracer of the gas associated with 595 continuum cores across the 15 protoclusters, providing the first estimates of the core systemic velocities and linewidths within the sample. We find that DCN (3-2) is detected towards a higher percentage of cores in evolved regions than the young and intermediate-stage protoclusters and is likely a more complete tracer of the core population in more evolved protoclusters. The full ALMA 12m-array cubes for the ALMA-IMF Large Program are provided with this DR1 release. Fil: Cunningham, N.. Universite Grenoble Alpes; Francia Fil: Ginsburg, A.. University of Florida; Estados Unidos Fil: Galván Madrid, R.. No especifíca; Fil: Motte, F.. Universite Grenoble Alpes; Francia Fil: Csengeri, T.. Universite de Bordeaux; Francia Fil: Stutz, A. M.. Universidad de Concepción; Chile 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: Álvarez Gutiérrez, R. H.. Universidad de Concepción; Chile Fil: Armante, M.. Universite de Bordeaux; Francia Fil: Baug, T.. Bose National Centre For Basic Sciences; India Fil: Bonfand, M.. Ecole Normale Supérieure; Francia Fil: Bontemps, Sophie. Universite de Bordeaux; Francia Fil: Braine, J.. Universite de Bordeaux; Francia Fil: Brouillet, N.. Universite de Bordeaux; Francia Fil: Busquets, Gabriel. Universidad de Barcelona; España Fil: Díaz González, D. J.. Instituto de Radioastronomía y Astrofísica; México Fil: Di Francesco, J.. National Research Council Of Canada; Canadá Fil: Gusdorf, A.. Universite de Bordeaux; Francia Fil: Herpin, F.. Ecole Normale Supérieure; Francia Fil: Liu, H.. Yunnan University; China Fil: López-Sepulcre, A.. Universite Grenoble Alpes; Francia Fil: Louvet, F.. Universite Grenoble Alpes; Francia Fil: Lu, X.. Chinese Academy of Sciences; República de China Fil: Maud, L.. European Southern Observatory; Alemania Fil: Nony, T.. Instituto de Radioastronomía y Astrofísica; México Fil: Olguin, F. A.. National Tsing Hua University; China Fil: Pouteau, Y.. Universite Grenoble Alpes; Francia Fil: Rivera Soto, R.. Instituto de Radioastronomía y Astrofísica; México Fil: Sandoval Garrido, N. A.. Universidad de Concepción; Chile Fil: Sanhueza, P.. National Astronomical Observatory Of Japan; Japón Fil: Tatematsu, K.. National Astronomical Observatory Of Japan; Japón Fil: Towner, A. P. M.. University of Florida; Estados Unidos Fil: Valeille Manet, M.. Universite de Bordeaux; Francia |
| description |
ALMA-IMF is an Atacama Large Millimeter/submillimeter Array (ALMA) Large Program designed to measure the core mass function (CMF) of 15 protoclusters chosen to span their early evolutionary stages. It further aims to understand their kinematics, chemistry, and the impact of gas inflow, accretion, and dynamics on the CMF. We present here the first release of the ALMA-IMF line data cubes (DR1), produced from the combination of two ALMA 12 m-array configurations. The data include 12 spectral windows, with eight at 1.3 mm and four at 3 mm. The broad spectral coverage of ALMA-IMF (∼6.7 GHz bandwidth coverage per field) hosts a wealth of simple atomic, molecular, ionised, and complex organic molecular lines. We describe the line cube calibration done by ALMA and the subsequent calibration and imaging we performed. We discuss our choice of calibration parameters and optimisation of the cleaning parameters, and we demonstrate the utility and necessity of additional processing compared to the ALMA archive pipeline. As a demonstration of the scientific potential of these data, we present a first analysis of the DCN (3-2) line. We find that DCN (3-2) traces a diversity of morphologies and complex velocity structures, which tend to be more filamentary and widespread in evolved regions and are more compact in the young and intermediate-stage protoclusters. Furthermore, we used the DCN (3-2) emission as a tracer of the gas associated with 595 continuum cores across the 15 protoclusters, providing the first estimates of the core systemic velocities and linewidths within the sample. We find that DCN (3-2) is detected towards a higher percentage of cores in evolved regions than the young and intermediate-stage protoclusters and is likely a more complete tracer of the core population in more evolved protoclusters. The full ALMA 12m-array cubes for the ALMA-IMF Large Program are provided with this DR1 release. |
| publishDate |
2023 |
| dc.date.none.fl_str_mv |
2023-10 |
| 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/11336/251916 Cunningham, N.; Ginsburg, A.; Galván Madrid, R.; Motte, F.; Csengeri, T.; et al.; ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2); EDP Sciences; Astronomy and Astrophysics; 678; 10-2023; 1-73 0004-6361 CONICET Digital CONICET |
| url |
http://hdl.handle.net/11336/251916 |
| identifier_str_mv |
Cunningham, N.; Ginsburg, A.; Galván Madrid, R.; Motte, F.; Csengeri, T.; et al.; ALMA-IMF. VII. First release of the full spectral line cubes: Core kinematics traced by DCN J = (3−2); EDP Sciences; Astronomy and Astrophysics; 678; 10-2023; 1-73 0004-6361 CONICET Digital CONICET |
| dc.language.none.fl_str_mv |
eng |
| language |
eng |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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EDP Sciences |
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EDP Sciences |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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