Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs
- Autores
- Vazzano, María Mercedes; Fernandez Lopez, Manuel; Plunkett, Adele; de Gregorio Monsalvo, Itziar; Santamaría Miranda, Alejandro; Takahashi, Satoko; Lopez, Cristian
- Año de publicación
- 2021
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- By studying 7 objects in the Lupus clouds we aim to test if a coherence exists between commonly used evolutionary tracers. We present ALMA observations of the continuum and molecular line emission that probe the dense gas and dust of cores and their associated molecular outflows. Our source selection in a common environment allows for a consistent comparison across different evolutionary stages. The quality of the ALMA molecular data allows us to reveal the nature of the molecular outflows by studying their morphology and kinematics. The images in IRAS15398-3359 appear to show that it drives a precessing episodic jet-driven outflow with at least 4 ejections separated by periods of time between 50 and 80 years, while data in IRAS16059-3857 show similarities with a wide-angle wind model also showing signs of being episodic. The outflow of J160115-41523 could be better explain with the wide-angle wind model as well, but new observations are needed to explore its nature. We find that the most common evolutionary tracers are useful for broad evolutionary classifications, but are not consistent with each other to provide enough granularity to disentangle different evolutionary stage of sources that belong to the same Class. Outflow properties used as protostellar age tracers (mass, momentum, energy, opening angle) may suffer from differences in the nature of each outflow, thus detailed observations are needed to refine evolutionary classifications. We found both AzTEC-lup1-2 and AzTEC-lup3-5 to be in the pre-stellar stage, although the latter could be more evolved. IRAS15398-3359, IRAS16059-3857 and J160115-41523, which have clearly detected outflows, are Class 0 sources, although we are not able to determine which is younger and which is older. Sz102 and Merin28 are the most evolved sources and show signs of having associated flows, not as well traced by CO as for the younger sources.
Fil: Vazzano, María Mercedes. 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: 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: Plunkett, Adele. National Radio Astronomy Observatory; Estados Unidos
Fil: de Gregorio Monsalvo, Itziar. European Southern Observatory Chile.; Chile
Fil: Santamaría Miranda, Alejandro. European Southern Observatory Chile.; Chile
Fil: Takahashi, Satoko. Joint Alma Observatory; Chile
Fil: Lopez, Cristian. Joint Alma Observatory; Chile - Materia
-
STAR: FORMATION
ISM: MOLECULES
ISM: JETS AND OUTFLOWS - 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:11336/135284
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Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOsVazzano, María MercedesFernandez Lopez, ManuelPlunkett, Adelede Gregorio Monsalvo, ItziarSantamaría Miranda, AlejandroTakahashi, SatokoLopez, CristianSTAR: FORMATIONISM: MOLECULESISM: JETS AND OUTFLOWShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1By studying 7 objects in the Lupus clouds we aim to test if a coherence exists between commonly used evolutionary tracers. We present ALMA observations of the continuum and molecular line emission that probe the dense gas and dust of cores and their associated molecular outflows. Our source selection in a common environment allows for a consistent comparison across different evolutionary stages. The quality of the ALMA molecular data allows us to reveal the nature of the molecular outflows by studying their morphology and kinematics. The images in IRAS15398-3359 appear to show that it drives a precessing episodic jet-driven outflow with at least 4 ejections separated by periods of time between 50 and 80 years, while data in IRAS16059-3857 show similarities with a wide-angle wind model also showing signs of being episodic. The outflow of J160115-41523 could be better explain with the wide-angle wind model as well, but new observations are needed to explore its nature. We find that the most common evolutionary tracers are useful for broad evolutionary classifications, but are not consistent with each other to provide enough granularity to disentangle different evolutionary stage of sources that belong to the same Class. Outflow properties used as protostellar age tracers (mass, momentum, energy, opening angle) may suffer from differences in the nature of each outflow, thus detailed observations are needed to refine evolutionary classifications. We found both AzTEC-lup1-2 and AzTEC-lup3-5 to be in the pre-stellar stage, although the latter could be more evolved. IRAS15398-3359, IRAS16059-3857 and J160115-41523, which have clearly detected outflows, are Class 0 sources, although we are not able to determine which is younger and which is older. Sz102 and Merin28 are the most evolved sources and show signs of having associated flows, not as well traced by CO as for the younger sources.Fil: Vazzano, María Mercedes. 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: 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: Plunkett, Adele. National Radio Astronomy Observatory; Estados UnidosFil: de Gregorio Monsalvo, Itziar. European Southern Observatory Chile.; ChileFil: Santamaría Miranda, Alejandro. European Southern Observatory Chile.; ChileFil: Takahashi, Satoko. Joint Alma Observatory; ChileFil: Lopez, Cristian. Joint Alma Observatory; ChileEDP Sciences2021-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/135284Vazzano, María Mercedes; Fernandez Lopez, Manuel; Plunkett, Adele; de Gregorio Monsalvo, Itziar; Santamaría Miranda, Alejandro; et al.; Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs; EDP Sciences; Astronomy and Astrophysics; 648; A41; 4-2021; 1-380004-6361CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://www.aanda.org/articles/aa/abs/2021/04/aa39228-20/aa39228-20.htmlinfo:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1051/0004-6361/202039228info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:21:31Zoai:ri.conicet.gov.ar:11336/135284instacron: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 10:21:31.538CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
title |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
spellingShingle |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs Vazzano, María Mercedes STAR: FORMATION ISM: MOLECULES ISM: JETS AND OUTFLOWS |
title_short |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
title_full |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
title_fullStr |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
title_full_unstemmed |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
title_sort |
Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs |
dc.creator.none.fl_str_mv |
Vazzano, María Mercedes Fernandez Lopez, Manuel Plunkett, Adele de Gregorio Monsalvo, Itziar Santamaría Miranda, Alejandro Takahashi, Satoko Lopez, Cristian |
author |
Vazzano, María Mercedes |
author_facet |
Vazzano, María Mercedes Fernandez Lopez, Manuel Plunkett, Adele de Gregorio Monsalvo, Itziar Santamaría Miranda, Alejandro Takahashi, Satoko Lopez, Cristian |
author_role |
author |
author2 |
Fernandez Lopez, Manuel Plunkett, Adele de Gregorio Monsalvo, Itziar Santamaría Miranda, Alejandro Takahashi, Satoko Lopez, Cristian |
author2_role |
author author author author author author |
dc.subject.none.fl_str_mv |
STAR: FORMATION ISM: MOLECULES ISM: JETS AND OUTFLOWS |
topic |
STAR: FORMATION ISM: MOLECULES ISM: JETS AND OUTFLOWS |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
By studying 7 objects in the Lupus clouds we aim to test if a coherence exists between commonly used evolutionary tracers. We present ALMA observations of the continuum and molecular line emission that probe the dense gas and dust of cores and their associated molecular outflows. Our source selection in a common environment allows for a consistent comparison across different evolutionary stages. The quality of the ALMA molecular data allows us to reveal the nature of the molecular outflows by studying their morphology and kinematics. The images in IRAS15398-3359 appear to show that it drives a precessing episodic jet-driven outflow with at least 4 ejections separated by periods of time between 50 and 80 years, while data in IRAS16059-3857 show similarities with a wide-angle wind model also showing signs of being episodic. The outflow of J160115-41523 could be better explain with the wide-angle wind model as well, but new observations are needed to explore its nature. We find that the most common evolutionary tracers are useful for broad evolutionary classifications, but are not consistent with each other to provide enough granularity to disentangle different evolutionary stage of sources that belong to the same Class. Outflow properties used as protostellar age tracers (mass, momentum, energy, opening angle) may suffer from differences in the nature of each outflow, thus detailed observations are needed to refine evolutionary classifications. We found both AzTEC-lup1-2 and AzTEC-lup3-5 to be in the pre-stellar stage, although the latter could be more evolved. IRAS15398-3359, IRAS16059-3857 and J160115-41523, which have clearly detected outflows, are Class 0 sources, although we are not able to determine which is younger and which is older. Sz102 and Merin28 are the most evolved sources and show signs of having associated flows, not as well traced by CO as for the younger sources. Fil: Vazzano, María Mercedes. 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: 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: Plunkett, Adele. National Radio Astronomy Observatory; Estados Unidos Fil: de Gregorio Monsalvo, Itziar. European Southern Observatory Chile.; Chile Fil: Santamaría Miranda, Alejandro. European Southern Observatory Chile.; Chile Fil: Takahashi, Satoko. Joint Alma Observatory; Chile Fil: Lopez, Cristian. Joint Alma Observatory; Chile |
description |
By studying 7 objects in the Lupus clouds we aim to test if a coherence exists between commonly used evolutionary tracers. We present ALMA observations of the continuum and molecular line emission that probe the dense gas and dust of cores and their associated molecular outflows. Our source selection in a common environment allows for a consistent comparison across different evolutionary stages. The quality of the ALMA molecular data allows us to reveal the nature of the molecular outflows by studying their morphology and kinematics. The images in IRAS15398-3359 appear to show that it drives a precessing episodic jet-driven outflow with at least 4 ejections separated by periods of time between 50 and 80 years, while data in IRAS16059-3857 show similarities with a wide-angle wind model also showing signs of being episodic. The outflow of J160115-41523 could be better explain with the wide-angle wind model as well, but new observations are needed to explore its nature. We find that the most common evolutionary tracers are useful for broad evolutionary classifications, but are not consistent with each other to provide enough granularity to disentangle different evolutionary stage of sources that belong to the same Class. Outflow properties used as protostellar age tracers (mass, momentum, energy, opening angle) may suffer from differences in the nature of each outflow, thus detailed observations are needed to refine evolutionary classifications. We found both AzTEC-lup1-2 and AzTEC-lup3-5 to be in the pre-stellar stage, although the latter could be more evolved. IRAS15398-3359, IRAS16059-3857 and J160115-41523, which have clearly detected outflows, are Class 0 sources, although we are not able to determine which is younger and which is older. Sz102 and Merin28 are the most evolved sources and show signs of having associated flows, not as well traced by CO as for the younger sources. |
publishDate |
2021 |
dc.date.none.fl_str_mv |
2021-04 |
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/11336/135284 Vazzano, María Mercedes; Fernandez Lopez, Manuel; Plunkett, Adele; de Gregorio Monsalvo, Itziar; Santamaría Miranda, Alejandro; et al.; Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs; EDP Sciences; Astronomy and Astrophysics; 648; A41; 4-2021; 1-38 0004-6361 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/135284 |
identifier_str_mv |
Vazzano, María Mercedes; Fernandez Lopez, Manuel; Plunkett, Adele; de Gregorio Monsalvo, Itziar; Santamaría Miranda, Alejandro; et al.; Outflows, envelopes, and disks as evolutionary indicators in Lupus YSOs; EDP Sciences; Astronomy and Astrophysics; 648; A41; 4-2021; 1-38 0004-6361 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://www.aanda.org/articles/aa/abs/2021/04/aa39228-20/aa39228-20.html info:eu-repo/semantics/altIdentifier/url/https://doi.org/10.1051/0004-6361/202039228 |
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 application/pdf |
dc.publisher.none.fl_str_mv |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
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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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13.070432 |