Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South

Autores
Lee, Katherine; Mundy, Lee G.; Fernandez Lopez, Manuel; Storm, Shaye; Looney, Leslie; Segura Cox, Dominique; Teuben, Peter J.; Rosolowsky, Erik; Arce, Hector G.; Shirley, Yancy L.; Plunkett, Adele; Isella, Andrea; Tobin, John J.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
documento de conferencia
Estado
versión publicada
Descripción
We present a study of filaments in Serpens Main and Serpens South cluster regions based on N2H+(1-0) observations from the CARMA Large Area Star-formation Survey (CLASSy) and dust continuum images from the Herschel Space Observatory. Serpens Main and Serpens South are active star formation regions with prominent filamentary structures; however, the role of the filaments in the cluster formation is unclear. This study of filament structure and kinematics with high-angular resolution data (7 arcsecs), particularly in revealing possible infall signatures, provides physical insight to this question. Using the Herschel data, we estimate the temperature in and along filaments for comparison with their gas kinematics, spatial distribution, and N2H+(1-0) emission, to better understand their role in current star formation activities.
Fil: Lee, Katherine. University of Maryland; Estados Unidos
Fil: Mundy, Lee G.. University of Maryland; 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: Storm, Shaye. University of Maryland; Estados Unidos
Fil: Looney, Leslie. University of Illinois at Urbana- Champaign; Estados Unidos
Fil: Segura Cox, Dominique. University of Maryland; Estados Unidos
Fil: Teuben, Peter J.. University of Maryland; Estados Unidos
Fil: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Arce, Hector G.. Yale University; Estados Unidos
Fil: Shirley, Yancy L.. University of Arizona; Estados Unidos
Fil: Plunkett, Adele. Yale University; Estados Unidos
Fil: Isella, Andrea. Caltech; Estados Unidos
Fil: Tobin, John J.. National Radio Astronomy Observatory; Estados Unidos
223th meeting of the American Astronomical Society
Washington
Estados Unidos
American Astronomical Society
Materia
MOLECULAR CLOUDS
STAR FORMATION
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:11336/139855
Acceder
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network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens SouthLee, KatherineMundy, Lee G.Fernandez Lopez, ManuelStorm, ShayeLooney, LeslieSegura Cox, DominiqueTeuben, Peter J.Rosolowsky, ErikArce, Hector G.Shirley, Yancy L.Plunkett, AdeleIsella, AndreaTobin, John J.MOLECULAR CLOUDSSTAR FORMATIONhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a study of filaments in Serpens Main and Serpens South cluster regions based on N2H+(1-0) observations from the CARMA Large Area Star-formation Survey (CLASSy) and dust continuum images from the Herschel Space Observatory. Serpens Main and Serpens South are active star formation regions with prominent filamentary structures; however, the role of the filaments in the cluster formation is unclear. This study of filament structure and kinematics with high-angular resolution data (7 arcsecs), particularly in revealing possible infall signatures, provides physical insight to this question. Using the Herschel data, we estimate the temperature in and along filaments for comparison with their gas kinematics, spatial distribution, and N2H+(1-0) emission, to better understand their role in current star formation activities.Fil: Lee, Katherine. University of Maryland; Estados UnidosFil: Mundy, Lee G.. University of Maryland; 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: Storm, Shaye. University of Maryland; Estados UnidosFil: Looney, Leslie. University of Illinois at Urbana- Champaign; Estados UnidosFil: Segura Cox, Dominique. University of Maryland; Estados UnidosFil: Teuben, Peter J.. University of Maryland; Estados UnidosFil: Rosolowsky, Erik. University of Alberta; CanadáFil: Arce, Hector G.. Yale University; Estados UnidosFil: Shirley, Yancy L.. University of Arizona; Estados UnidosFil: Plunkett, Adele. Yale University; Estados UnidosFil: Isella, Andrea. Caltech; Estados UnidosFil: Tobin, John J.. National Radio Astronomy Observatory; Estados Unidos223th meeting of the American Astronomical SocietyWashingtonEstados UnidosAmerican Astronomical SocietyAmerican Astronomical Society2014info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectReuniónJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/139855Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South; 223th meeting of the American Astronomical Society; Washington; Estados Unidos; 2014; 366-3660002-75372330-9458CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://aas.org/sites/default/files/2020-01/AAS_223_Abstracts.pdfNacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:08:05Zoai:ri.conicet.gov.ar:11336/139855instacron: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 10:08:05.984CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
title Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
spellingShingle Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
Lee, Katherine
MOLECULAR CLOUDS
STAR FORMATION
title_short Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
title_full Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
title_fullStr Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
title_full_unstemmed Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
title_sort Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South
dc.creator.none.fl_str_mv Lee, Katherine
Mundy, Lee G.
Fernandez Lopez, Manuel
Storm, Shaye
Looney, Leslie
Segura Cox, Dominique
Teuben, Peter J.
Rosolowsky, Erik
Arce, Hector G.
Shirley, Yancy L.
Plunkett, Adele
Isella, Andrea
Tobin, John J.
author Lee, Katherine
author_facet Lee, Katherine
Mundy, Lee G.
Fernandez Lopez, Manuel
Storm, Shaye
Looney, Leslie
Segura Cox, Dominique
Teuben, Peter J.
Rosolowsky, Erik
Arce, Hector G.
Shirley, Yancy L.
Plunkett, Adele
Isella, Andrea
Tobin, John J.
author_role author
author2 Mundy, Lee G.
Fernandez Lopez, Manuel
Storm, Shaye
Looney, Leslie
Segura Cox, Dominique
Teuben, Peter J.
Rosolowsky, Erik
Arce, Hector G.
Shirley, Yancy L.
Plunkett, Adele
Isella, Andrea
Tobin, John J.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv MOLECULAR CLOUDS
STAR FORMATION
topic MOLECULAR CLOUDS
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 a study of filaments in Serpens Main and Serpens South cluster regions based on N2H+(1-0) observations from the CARMA Large Area Star-formation Survey (CLASSy) and dust continuum images from the Herschel Space Observatory. Serpens Main and Serpens South are active star formation regions with prominent filamentary structures; however, the role of the filaments in the cluster formation is unclear. This study of filament structure and kinematics with high-angular resolution data (7 arcsecs), particularly in revealing possible infall signatures, provides physical insight to this question. Using the Herschel data, we estimate the temperature in and along filaments for comparison with their gas kinematics, spatial distribution, and N2H+(1-0) emission, to better understand their role in current star formation activities.
Fil: Lee, Katherine. University of Maryland; Estados Unidos
Fil: Mundy, Lee G.. University of Maryland; 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: Storm, Shaye. University of Maryland; Estados Unidos
Fil: Looney, Leslie. University of Illinois at Urbana- Champaign; Estados Unidos
Fil: Segura Cox, Dominique. University of Maryland; Estados Unidos
Fil: Teuben, Peter J.. University of Maryland; Estados Unidos
Fil: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Arce, Hector G.. Yale University; Estados Unidos
Fil: Shirley, Yancy L.. University of Arizona; Estados Unidos
Fil: Plunkett, Adele. Yale University; Estados Unidos
Fil: Isella, Andrea. Caltech; Estados Unidos
Fil: Tobin, John J.. National Radio Astronomy Observatory; Estados Unidos
223th meeting of the American Astronomical Society
Washington
Estados Unidos
American Astronomical Society
description We present a study of filaments in Serpens Main and Serpens South cluster regions based on N2H+(1-0) observations from the CARMA Large Area Star-formation Survey (CLASSy) and dust continuum images from the Herschel Space Observatory. Serpens Main and Serpens South are active star formation regions with prominent filamentary structures; however, the role of the filaments in the cluster formation is unclear. This study of filament structure and kinematics with high-angular resolution data (7 arcsecs), particularly in revealing possible infall signatures, provides physical insight to this question. Using the Herschel data, we estimate the temperature in and along filaments for comparison with their gas kinematics, spatial distribution, and N2H+(1-0) emission, to better understand their role in current star formation activities.
publishDate 2014
dc.date.none.fl_str_mv 2014
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/11336/139855
Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South; 223th meeting of the American Astronomical Society; Washington; Estados Unidos; 2014; 366-366
0002-7537
2330-9458
CONICET Digital
CONICET
url http://hdl.handle.net/11336/139855
identifier_str_mv Kinematics and Temperature Structures of Filaments in Serpens Main and Serpens South; 223th meeting of the American Astronomical Society; Washington; Estados Unidos; 2014; 366-366
0002-7537
2330-9458
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://aas.org/sites/default/files/2020-01/AAS_223_Abstracts.pdf
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.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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score 13.070432

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