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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/251900
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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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1844613879161683968 |
score |
13.070432 |