Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar

Autores
Fernandez Lopez, Manuel; Girart, J. M.; López Vázquez, J. A.; Estalella, R.; Busquets, Gabriel; Curiel, S.; Añez López, N.
Año de publicación
2023
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present new Atacama Large Millimeter/submillimeter Array 0.98 mm observations of the continuum emission and several molecular lines toward the high-mass protostellar system GGD 27-MM1, driving the HH 80-81 radio jet. The detailed analysis of the continuum and the CH3CN molecular emission allows us to separate the contributions from the dust content of the disk (extending up to 190 au), the molecular content of the disk (extending from 140–360 au), and the content of the envelope, revealing the presence of several possible accretion streamers (also seen in other molecular tracers, such as CH3OH). We analyze the physical properties of the system, producing temperature and column density maps, and radial profiles for the disk and the envelope. We qualitatively reproduce the trajectories and line-of-sight velocities of the possible streamers using a theoretical model approach. An ad hoc model of a flared disk comprising a hot dust disk embedded in cold gas fits the H2S emission, which revealed the molecular disk as a crescent shape with a prominent central absorption. Another fit to the central absorption spectrum suggests that the absorption is probably caused by different external cold layers from the envelope or the accretion streamers. Finally, the analysis of the rotation pattern of the different molecular transitions in the molecular disk suggests that there is an inner zone devoid of molecular content.
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: Girart, J. M.. Instituto de Ciencias del Espacio; España
Fil: López Vázquez, J. A.. Academia Sinica Institute of Astronomy and Astrophysics; China
Fil: Estalella, R.. Universidad de Barcelona; España
Fil: Busquets, Gabriel. Universidad de Barcelona; España
Fil: Curiel, S.. Universidad Nacional Autónoma de México; México
Fil: Añez López, N.. Universite Paris Saclay; Francia. Universite Paris-Saclay ;
Materia
Interstellar molecules
Young stellar objects
Protostars
Interstellar medium
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:11336/251900

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spelling Disk and Envelope Streamers of the GGD 27-MM1 Massive ProtostarFernandez Lopez, ManuelGirart, J. M.López Vázquez, J. A.Estalella, R.Busquets, GabrielCuriel, S.Añez López, N.Interstellar moleculesYoung stellar objectsProtostarsInterstellar mediumhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present new Atacama Large Millimeter/submillimeter Array 0.98 mm observations of the continuum emission and several molecular lines toward the high-mass protostellar system GGD 27-MM1, driving the HH 80-81 radio jet. The detailed analysis of the continuum and the CH3CN molecular emission allows us to separate the contributions from the dust content of the disk (extending up to 190 au), the molecular content of the disk (extending from 140–360 au), and the content of the envelope, revealing the presence of several possible accretion streamers (also seen in other molecular tracers, such as CH3OH). We analyze the physical properties of the system, producing temperature and column density maps, and radial profiles for the disk and the envelope. We qualitatively reproduce the trajectories and line-of-sight velocities of the possible streamers using a theoretical model approach. An ad hoc model of a flared disk comprising a hot dust disk embedded in cold gas fits the H2S emission, which revealed the molecular disk as a crescent shape with a prominent central absorption. Another fit to the central absorption spectrum suggests that the absorption is probably caused by different external cold layers from the envelope or the accretion streamers. Finally, the analysis of the rotation pattern of the different molecular transitions in the molecular disk suggests that there is an inner zone devoid of molecular content.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; ArgentinaFil: Girart, J. M.. Instituto de Ciencias del Espacio; EspañaFil: López Vázquez, J. A.. Academia Sinica Institute of Astronomy and Astrophysics; ChinaFil: Estalella, R.. Universidad de Barcelona; EspañaFil: Busquets, Gabriel. Universidad de Barcelona; EspañaFil: Curiel, S.. Universidad Nacional Autónoma de México; MéxicoFil: Añez López, N.. Universite Paris Saclay; Francia. Universite Paris-Saclay ;IOP Publishing2023-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/251900Fernandez Lopez, Manuel; Girart, J. M.; López Vázquez, J. A.; Estalella, R.; Busquets, Gabriel; et al.; Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar; IOP Publishing; Astrophysical Journal; 956; 2; 10-2023; 1-360004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ace786info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ace786info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:04:54Zoai:ri.conicet.gov.ar:11336/251900instacron: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 10:04:54.888CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
title Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
spellingShingle Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
Fernandez Lopez, Manuel
Interstellar molecules
Young stellar objects
Protostars
Interstellar medium
title_short Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
title_full Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
title_fullStr Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
title_full_unstemmed Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
title_sort Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar
dc.creator.none.fl_str_mv Fernandez Lopez, Manuel
Girart, J. M.
López Vázquez, J. A.
Estalella, R.
Busquets, Gabriel
Curiel, S.
Añez López, N.
author Fernandez Lopez, Manuel
author_facet Fernandez Lopez, Manuel
Girart, J. M.
López Vázquez, J. A.
Estalella, R.
Busquets, Gabriel
Curiel, S.
Añez López, N.
author_role author
author2 Girart, J. M.
López Vázquez, J. A.
Estalella, R.
Busquets, Gabriel
Curiel, S.
Añez López, N.
author2_role author
author
author
author
author
author
dc.subject.none.fl_str_mv Interstellar molecules
Young stellar objects
Protostars
Interstellar medium
topic Interstellar molecules
Young stellar objects
Protostars
Interstellar medium
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 new Atacama Large Millimeter/submillimeter Array 0.98 mm observations of the continuum emission and several molecular lines toward the high-mass protostellar system GGD 27-MM1, driving the HH 80-81 radio jet. The detailed analysis of the continuum and the CH3CN molecular emission allows us to separate the contributions from the dust content of the disk (extending up to 190 au), the molecular content of the disk (extending from 140–360 au), and the content of the envelope, revealing the presence of several possible accretion streamers (also seen in other molecular tracers, such as CH3OH). We analyze the physical properties of the system, producing temperature and column density maps, and radial profiles for the disk and the envelope. We qualitatively reproduce the trajectories and line-of-sight velocities of the possible streamers using a theoretical model approach. An ad hoc model of a flared disk comprising a hot dust disk embedded in cold gas fits the H2S emission, which revealed the molecular disk as a crescent shape with a prominent central absorption. Another fit to the central absorption spectrum suggests that the absorption is probably caused by different external cold layers from the envelope or the accretion streamers. Finally, the analysis of the rotation pattern of the different molecular transitions in the molecular disk suggests that there is an inner zone devoid of molecular content.
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: Girart, J. M.. Instituto de Ciencias del Espacio; España
Fil: López Vázquez, J. A.. Academia Sinica Institute of Astronomy and Astrophysics; China
Fil: Estalella, R.. Universidad de Barcelona; España
Fil: Busquets, Gabriel. Universidad de Barcelona; España
Fil: Curiel, S.. Universidad Nacional Autónoma de México; México
Fil: Añez López, N.. Universite Paris Saclay; Francia. Universite Paris-Saclay ;
description We present new Atacama Large Millimeter/submillimeter Array 0.98 mm observations of the continuum emission and several molecular lines toward the high-mass protostellar system GGD 27-MM1, driving the HH 80-81 radio jet. The detailed analysis of the continuum and the CH3CN molecular emission allows us to separate the contributions from the dust content of the disk (extending up to 190 au), the molecular content of the disk (extending from 140–360 au), and the content of the envelope, revealing the presence of several possible accretion streamers (also seen in other molecular tracers, such as CH3OH). We analyze the physical properties of the system, producing temperature and column density maps, and radial profiles for the disk and the envelope. We qualitatively reproduce the trajectories and line-of-sight velocities of the possible streamers using a theoretical model approach. An ad hoc model of a flared disk comprising a hot dust disk embedded in cold gas fits the H2S emission, which revealed the molecular disk as a crescent shape with a prominent central absorption. Another fit to the central absorption spectrum suggests that the absorption is probably caused by different external cold layers from the envelope or the accretion streamers. Finally, the analysis of the rotation pattern of the different molecular transitions in the molecular disk suggests that there is an inner zone devoid of molecular content.
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/11336/251900
Fernandez Lopez, Manuel; Girart, J. M.; López Vázquez, J. A.; Estalella, R.; Busquets, Gabriel; et al.; Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar; IOP Publishing; Astrophysical Journal; 956; 2; 10-2023; 1-36
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/251900
identifier_str_mv Fernandez Lopez, Manuel; Girart, J. M.; López Vázquez, J. A.; Estalella, R.; Busquets, Gabriel; et al.; Disk and Envelope Streamers of the GGD 27-MM1 Massive Protostar; IOP Publishing; Astrophysical Journal; 956; 2; 10-2023; 1-36
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/ace786
info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ace786
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)
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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