Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow
- Autores
- López Vázquez, J. A.; Lee, Chin Fei; Fernandez Lopez, Manuel; Louvet, Fabien; Guerra Alvarado, O.; Zapata, Luis A.
- Año de publicación
- 2024
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present archival Atacama Large Millimeter/submillimeter Array band 6 observations of the 13CO (J = 2–1) and 12CO (J = 2–1) molecular line emission of the protostellar system associated with HH 30. The 13CO molecular line shows the accretion disk while the molecular outflow is traced by the emission of the 12CO molecular line. We estimated a dynamical mass for the central object of 0.45 ± 0.14 M ⊙, and a mass for the molecular outflow of (1.83 ± 0.19) × 10‑4 M ⊙. The molecular outflow presents an internal cavity as well as multiple outflowing shell structures. We distinguish three different shells with constant expansion (∼4–6 km s‑1) and possible rotation signatures (≤0.5 km s‑1). We find that the shells can be explained by magnetocentrifugal disk winds with launching radii R launch ≲ 4 au and a small magnetic lever arm λ ∼ 1.6–1.9. The multiple shell structure may be the result of episodic ejections of the material from the accretion disk associated with three different epochs with dynamical ages of 497 ± 15 yr, 310 ± 9 yr, and 262 ± 11 yr for the first, second, and third shells, respectively. The outermost shell was ejected 187 ± 17 yr before the middle shell, while the middle shell was launched 48 ± 14 yr before the innermost shell. Our estimations of the linear and angular momentum rates of the outflow as well as the accretion luminosity are consistent with the values expected if the outflow of HH 30 is produced by a wide-angle disk wind.
Fil: López Vázquez, J. A.. Academia Sinica Institute of Astronomy and Astrophysics; China
Fil: Lee, Chin Fei. Academia Sinica Institute of Astronomy and Astrophysics; China
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: Louvet, Fabien. Universite Grenoble Alpes; Francia
Fil: Guerra Alvarado, O.. Leiden University; Países Bajos
Fil: Zapata, Luis A.. Universidad Nacional Autónoma de México; México - Materia
-
Accretion
Herbig-Haro objects
Star formation - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/267540
Ver los metadatos del registro completo
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Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 OutflowLópez Vázquez, J. A.Lee, Chin FeiFernandez Lopez, ManuelLouvet, FabienGuerra Alvarado, O.Zapata, Luis A.AccretionHerbig-Haro objectsStar formationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present archival Atacama Large Millimeter/submillimeter Array band 6 observations of the 13CO (J = 2–1) and 12CO (J = 2–1) molecular line emission of the protostellar system associated with HH 30. The 13CO molecular line shows the accretion disk while the molecular outflow is traced by the emission of the 12CO molecular line. We estimated a dynamical mass for the central object of 0.45 ± 0.14 M ⊙, and a mass for the molecular outflow of (1.83 ± 0.19) × 10‑4 M ⊙. The molecular outflow presents an internal cavity as well as multiple outflowing shell structures. We distinguish three different shells with constant expansion (∼4–6 km s‑1) and possible rotation signatures (≤0.5 km s‑1). We find that the shells can be explained by magnetocentrifugal disk winds with launching radii R launch ≲ 4 au and a small magnetic lever arm λ ∼ 1.6–1.9. The multiple shell structure may be the result of episodic ejections of the material from the accretion disk associated with three different epochs with dynamical ages of 497 ± 15 yr, 310 ± 9 yr, and 262 ± 11 yr for the first, second, and third shells, respectively. The outermost shell was ejected 187 ± 17 yr before the middle shell, while the middle shell was launched 48 ± 14 yr before the innermost shell. Our estimations of the linear and angular momentum rates of the outflow as well as the accretion luminosity are consistent with the values expected if the outflow of HH 30 is produced by a wide-angle disk wind.Fil: López Vázquez, J. A.. Academia Sinica Institute of Astronomy and Astrophysics; ChinaFil: Lee, Chin Fei. Academia Sinica Institute of Astronomy and Astrophysics; ChinaFil: 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: Louvet, Fabien. Universite Grenoble Alpes; FranciaFil: Guerra Alvarado, O.. Leiden University; Países BajosFil: Zapata, Luis A.. Universidad Nacional Autónoma de México; MéxicoIOP Publishing2024-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/267540López Vázquez, J. A.; Lee, Chin Fei; Fernandez Lopez, Manuel; Louvet, Fabien; Guerra Alvarado, O.; et al.; Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow; IOP Publishing; Astrophysical Journal; 962; 1; 2-2024; 1-170004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/ad132ainfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad132ainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:49:23Zoai:ri.conicet.gov.ar:11336/267540instacron: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 09:49:24.169CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
title |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
spellingShingle |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow López Vázquez, J. A. Accretion Herbig-Haro objects Star formation |
title_short |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
title_full |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
title_fullStr |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
title_full_unstemmed |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
title_sort |
Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow |
dc.creator.none.fl_str_mv |
López Vázquez, J. A. Lee, Chin Fei Fernandez Lopez, Manuel Louvet, Fabien Guerra Alvarado, O. Zapata, Luis A. |
author |
López Vázquez, J. A. |
author_facet |
López Vázquez, J. A. Lee, Chin Fei Fernandez Lopez, Manuel Louvet, Fabien Guerra Alvarado, O. Zapata, Luis A. |
author_role |
author |
author2 |
Lee, Chin Fei Fernandez Lopez, Manuel Louvet, Fabien Guerra Alvarado, O. Zapata, Luis A. |
author2_role |
author author author author author |
dc.subject.none.fl_str_mv |
Accretion Herbig-Haro objects Star formation |
topic |
Accretion Herbig-Haro objects Star formation |
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 archival Atacama Large Millimeter/submillimeter Array band 6 observations of the 13CO (J = 2–1) and 12CO (J = 2–1) molecular line emission of the protostellar system associated with HH 30. The 13CO molecular line shows the accretion disk while the molecular outflow is traced by the emission of the 12CO molecular line. We estimated a dynamical mass for the central object of 0.45 ± 0.14 M ⊙, and a mass for the molecular outflow of (1.83 ± 0.19) × 10‑4 M ⊙. The molecular outflow presents an internal cavity as well as multiple outflowing shell structures. We distinguish three different shells with constant expansion (∼4–6 km s‑1) and possible rotation signatures (≤0.5 km s‑1). We find that the shells can be explained by magnetocentrifugal disk winds with launching radii R launch ≲ 4 au and a small magnetic lever arm λ ∼ 1.6–1.9. The multiple shell structure may be the result of episodic ejections of the material from the accretion disk associated with three different epochs with dynamical ages of 497 ± 15 yr, 310 ± 9 yr, and 262 ± 11 yr for the first, second, and third shells, respectively. The outermost shell was ejected 187 ± 17 yr before the middle shell, while the middle shell was launched 48 ± 14 yr before the innermost shell. Our estimations of the linear and angular momentum rates of the outflow as well as the accretion luminosity are consistent with the values expected if the outflow of HH 30 is produced by a wide-angle disk wind. Fil: López Vázquez, J. A.. Academia Sinica Institute of Astronomy and Astrophysics; China Fil: Lee, Chin Fei. Academia Sinica Institute of Astronomy and Astrophysics; China 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: Louvet, Fabien. Universite Grenoble Alpes; Francia Fil: Guerra Alvarado, O.. Leiden University; Países Bajos Fil: Zapata, Luis A.. Universidad Nacional Autónoma de México; México |
description |
We present archival Atacama Large Millimeter/submillimeter Array band 6 observations of the 13CO (J = 2–1) and 12CO (J = 2–1) molecular line emission of the protostellar system associated with HH 30. The 13CO molecular line shows the accretion disk while the molecular outflow is traced by the emission of the 12CO molecular line. We estimated a dynamical mass for the central object of 0.45 ± 0.14 M ⊙, and a mass for the molecular outflow of (1.83 ± 0.19) × 10‑4 M ⊙. The molecular outflow presents an internal cavity as well as multiple outflowing shell structures. We distinguish three different shells with constant expansion (∼4–6 km s‑1) and possible rotation signatures (≤0.5 km s‑1). We find that the shells can be explained by magnetocentrifugal disk winds with launching radii R launch ≲ 4 au and a small magnetic lever arm λ ∼ 1.6–1.9. The multiple shell structure may be the result of episodic ejections of the material from the accretion disk associated with three different epochs with dynamical ages of 497 ± 15 yr, 310 ± 9 yr, and 262 ± 11 yr for the first, second, and third shells, respectively. The outermost shell was ejected 187 ± 17 yr before the middle shell, while the middle shell was launched 48 ± 14 yr before the innermost shell. Our estimations of the linear and angular momentum rates of the outflow as well as the accretion luminosity are consistent with the values expected if the outflow of HH 30 is produced by a wide-angle disk wind. |
publishDate |
2024 |
dc.date.none.fl_str_mv |
2024-02 |
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/11336/267540 López Vázquez, J. A.; Lee, Chin Fei; Fernandez Lopez, Manuel; Louvet, Fabien; Guerra Alvarado, O.; et al.; Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow; IOP Publishing; Astrophysical Journal; 962; 1; 2-2024; 1-17 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/267540 |
identifier_str_mv |
López Vázquez, J. A.; Lee, Chin Fei; Fernandez Lopez, Manuel; Louvet, Fabien; Guerra Alvarado, O.; et al.; Multiple Shells Driven by Disk Winds: ALMA Observations in the HH 30 Outflow; IOP Publishing; Astrophysical Journal; 962; 1; 2-2024; 1-17 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/ad132a info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ad132a |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by/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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1844613529466830848 |
score |
13.070432 |