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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/135284
Acceder
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network_name_str CONICET Digital (CONICET)
spelling 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 Técnicas2025-10-22T11:54:17Zoai: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:34982025-10-22 11:54:17.308CONICET 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
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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score 12.982451

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