ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South

Autores
Garces, Juan; Plunkett, Adele; Fernandez Lopez, Manuel; Arce, Héctor
Año de publicación
2021
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
Protostellar sources are characterized by continuum emission, as well as molecular emission tracing the gaseous envelope. The morphology and kinematics of the envelope are useful to study physical characteristics of protostellar candidates and their evolution, revealing aspects of the still unknown process of star formation. Our aim is to study protostars within the very young, active, and relatively nearby Serpens South cluster by analyzing their dense C18O envelopes/disks, enhancing the continuum source census of Plunkett et al. (2018). Most of these sources lie within a predominant filamentary structure. 67 protostellar candidates have been identified as continuum and/or IR sources, and the C18O data have been imaged by combining ALMA 12m-array, 7m-array, and single dish observations. The C18O spectra were organized in different groups according to their spectral shape and intensity. Also, given the fact that this region is embedded in a filamentary structure, we have made attempts to identify the level of line emission contribution that is most probably due to the filament instead of the source candidate itself. Finally, ongoing work will investigate possible trends associated to mass distribution among the filament, relations between source class, mass and C18O intensity, and different kinematic models to fit the envelopes´ motions.
Fil: Garces, Juan. Universidad Técnica Federico Santa María; Chile
Fil: Plunkett, Adele. National Radio Astronomy Observatory; Estados Unidos
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: Arce, Héctor. University of Yale; Estados Unidos
237th meeting of the American Astronomical Society
Estados Unidos
America Astronomical Society
Materia
Stars: formation
ISM: molecular
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:11336/139086
Acceder
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spelling ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens SouthGarces, JuanPlunkett, AdeleFernandez Lopez, ManuelArce, HéctorStars: formationISM: molecularhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Protostellar sources are characterized by continuum emission, as well as molecular emission tracing the gaseous envelope. The morphology and kinematics of the envelope are useful to study physical characteristics of protostellar candidates and their evolution, revealing aspects of the still unknown process of star formation. Our aim is to study protostars within the very young, active, and relatively nearby Serpens South cluster by analyzing their dense C18O envelopes/disks, enhancing the continuum source census of Plunkett et al. (2018). Most of these sources lie within a predominant filamentary structure. 67 protostellar candidates have been identified as continuum and/or IR sources, and the C18O data have been imaged by combining ALMA 12m-array, 7m-array, and single dish observations. The C18O spectra were organized in different groups according to their spectral shape and intensity. Also, given the fact that this region is embedded in a filamentary structure, we have made attempts to identify the level of line emission contribution that is most probably due to the filament instead of the source candidate itself. Finally, ongoing work will investigate possible trends associated to mass distribution among the filament, relations between source class, mass and C18O intensity, and different kinematic models to fit the envelopes´ motions.Fil: Garces, Juan. Universidad Técnica Federico Santa María; ChileFil: Plunkett, Adele. National Radio Astronomy Observatory; Estados UnidosFil: 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: Arce, Héctor. University of Yale; Estados Unidos237th meeting of the American Astronomical SocietyEstados UnidosAmerica Astronomical SocietyAmerican Astronomical Society2021info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectReuniónJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/139086ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South; 237th meeting of the American Astronomical Society; Estados Unidos; 2021; 1-160002-7537CONICET DigitalCONICETenghttps://ri.conicet.gov.ar/handle/11336/82426info:eu-repo/semantics/altIdentifier/url/https://baas.aas.org/pub/2021n1i143p04/release/1Nacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:19:01Zoai:ri.conicet.gov.ar:11336/139086instacron: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 10:19:01.641CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
title ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
spellingShingle ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
Garces, Juan
Stars: formation
ISM: molecular
title_short ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
title_full ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
title_fullStr ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
title_full_unstemmed ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
title_sort ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South
dc.creator.none.fl_str_mv Garces, Juan
Plunkett, Adele
Fernandez Lopez, Manuel
Arce, Héctor
author Garces, Juan
author_facet Garces, Juan
Plunkett, Adele
Fernandez Lopez, Manuel
Arce, Héctor
author_role author
author2 Plunkett, Adele
Fernandez Lopez, Manuel
Arce, Héctor
author2_role author
author
author
dc.subject.none.fl_str_mv Stars: formation
ISM: molecular
topic Stars: formation
ISM: molecular
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Protostellar sources are characterized by continuum emission, as well as molecular emission tracing the gaseous envelope. The morphology and kinematics of the envelope are useful to study physical characteristics of protostellar candidates and their evolution, revealing aspects of the still unknown process of star formation. Our aim is to study protostars within the very young, active, and relatively nearby Serpens South cluster by analyzing their dense C18O envelopes/disks, enhancing the continuum source census of Plunkett et al. (2018). Most of these sources lie within a predominant filamentary structure. 67 protostellar candidates have been identified as continuum and/or IR sources, and the C18O data have been imaged by combining ALMA 12m-array, 7m-array, and single dish observations. The C18O spectra were organized in different groups according to their spectral shape and intensity. Also, given the fact that this region is embedded in a filamentary structure, we have made attempts to identify the level of line emission contribution that is most probably due to the filament instead of the source candidate itself. Finally, ongoing work will investigate possible trends associated to mass distribution among the filament, relations between source class, mass and C18O intensity, and different kinematic models to fit the envelopes´ motions.
Fil: Garces, Juan. Universidad Técnica Federico Santa María; Chile
Fil: Plunkett, Adele. National Radio Astronomy Observatory; Estados Unidos
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: Arce, Héctor. University of Yale; Estados Unidos
237th meeting of the American Astronomical Society
Estados Unidos
America Astronomical Society
description Protostellar sources are characterized by continuum emission, as well as molecular emission tracing the gaseous envelope. The morphology and kinematics of the envelope are useful to study physical characteristics of protostellar candidates and their evolution, revealing aspects of the still unknown process of star formation. Our aim is to study protostars within the very young, active, and relatively nearby Serpens South cluster by analyzing their dense C18O envelopes/disks, enhancing the continuum source census of Plunkett et al. (2018). Most of these sources lie within a predominant filamentary structure. 67 protostellar candidates have been identified as continuum and/or IR sources, and the C18O data have been imaged by combining ALMA 12m-array, 7m-array, and single dish observations. The C18O spectra were organized in different groups according to their spectral shape and intensity. Also, given the fact that this region is embedded in a filamentary structure, we have made attempts to identify the level of line emission contribution that is most probably due to the filament instead of the source candidate itself. Finally, ongoing work will investigate possible trends associated to mass distribution among the filament, relations between source class, mass and C18O intensity, and different kinematic models to fit the envelopes´ motions.
publishDate 2021
dc.date.none.fl_str_mv 2021
dc.type.none.fl_str_mv info:eu-repo/semantics/publishedVersion
info:eu-repo/semantics/conferenceObject
Reunión
Journal
http://purl.org/coar/resource_type/c_5794
info:ar-repo/semantics/documentoDeConferencia
status_str publishedVersion
format conferenceObject
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/139086
ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South; 237th meeting of the American Astronomical Society; Estados Unidos; 2021; 1-16
0002-7537
CONICET Digital
CONICET
url http://hdl.handle.net/11336/139086
identifier_str_mv ALMA observations of gas and dust towards embedded protostellar envelopes in Serpens South; 237th meeting of the American Astronomical Society; Estados Unidos; 2021; 1-16
0002-7537
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv https://ri.conicet.gov.ar/handle/11336/82426
info:eu-repo/semantics/altIdentifier/url/https://baas.aas.org/pub/2021n1i143p04/release/1
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.coverage.none.fl_str_mv Nacional
dc.publisher.none.fl_str_mv American Astronomical Society
publisher.none.fl_str_mv American Astronomical Society
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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