Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451
- Autores
- Storm, Shaye; Mundy, Lee G.; Teuben, Peter J.; Lee, Katherine; Looney, Leslie; Fernandez Lopez, Manuel; Rosolowsky, Erik; Arce, Hector G.; Shirley, Yancy L.; Segura Cox, Dominique; Isella, Andrea; CLASSy Collaboration
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- We present spectral line maps of the dense gas across 400 square arcminutes of the Perseus Molecular Cloud, focused on NGC 1333, Barnard 1, and L1451. We constructed these maps as part of the CARMA Large Area Star-formation Survey (CLASSy), which is a CARMA key project that connects star forming cores to their natal cloud environment. This is achieved by leveraging CARMA's high angular resolution, imaging capability, and high efficiency at mosaicing large areas of the sky. CLASSy maps capture the structure and kinematics of N2H+, HCN, and HCO+ J=1-0 emission from thousand AU to parsec scales in three evolutionarily distinct regions of Perseus (in addition to two regions in Serpens). We show results from a non-binary dendrogram analysis of the Perseus N2H+ emission, which answers questions about the turbulent properties of the dense gas across evolutionary stages and across the range of size scales probed by CLASSy. There is a flat relation between mean internal turbulence and structure size for the dense gas in NGC 1333 and Barnard 1, but the magnitude of internal turbulence increases with nearby protostellar activity; the dense gas in the B1 main core and NGC 1333, which have active young stars, are characterized by mostly transonic to supersonic turbulence, while the filaments and clumps southwest of the B1 main core, which have no active young stars, have mostly subsonic turbulence. We have recently completed the observations of L1451, and results for that region will be revealed at the meeting. Released CLASSy data products can be found on our project website.
Fil: Storm, Shaye. University of Maryland; Estados Unidos
Fil: Mundy, Lee G.. University of Maryland; Estados Unidos
Fil: Teuben, Peter J.. University of Maryland; Estados Unidos
Fil: Lee, Katherine. University of Maryland; Estados Unidos
Fil: Looney, Leslie. University of Illinois at Urbana; 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: Rosolowsky, Erik. University of Alberta; Canadá
Fil: Arce, Hector G.. University of Yale; Estados Unidos
Fil: Shirley, Yancy L.. University of Arizona; Estados Unidos
Fil: Segura Cox, Dominique. University of Illinois; Estados Unidos
Fil: Isella, Andrea. Caltech; Estados Unidos
Fil: CLASSy Collaboration. No especifíca;
223rd American Astronomical Society Meeting
Washington
Estados Unidos
American Astronomical Society - Materia
- MOLECULAR CLOUDS
- 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:11336/141612
Ver los metadatos del registro completo
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CONICET Digital (CONICET) |
spelling |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451Storm, ShayeMundy, Lee G.Teuben, Peter J.Lee, KatherineLooney, LeslieFernandez Lopez, ManuelRosolowsky, ErikArce, Hector G.Shirley, Yancy L.Segura Cox, DominiqueIsella, AndreaCLASSy CollaborationMOLECULAR CLOUDShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present spectral line maps of the dense gas across 400 square arcminutes of the Perseus Molecular Cloud, focused on NGC 1333, Barnard 1, and L1451. We constructed these maps as part of the CARMA Large Area Star-formation Survey (CLASSy), which is a CARMA key project that connects star forming cores to their natal cloud environment. This is achieved by leveraging CARMA's high angular resolution, imaging capability, and high efficiency at mosaicing large areas of the sky. CLASSy maps capture the structure and kinematics of N2H+, HCN, and HCO+ J=1-0 emission from thousand AU to parsec scales in three evolutionarily distinct regions of Perseus (in addition to two regions in Serpens). We show results from a non-binary dendrogram analysis of the Perseus N2H+ emission, which answers questions about the turbulent properties of the dense gas across evolutionary stages and across the range of size scales probed by CLASSy. There is a flat relation between mean internal turbulence and structure size for the dense gas in NGC 1333 and Barnard 1, but the magnitude of internal turbulence increases with nearby protostellar activity; the dense gas in the B1 main core and NGC 1333, which have active young stars, are characterized by mostly transonic to supersonic turbulence, while the filaments and clumps southwest of the B1 main core, which have no active young stars, have mostly subsonic turbulence. We have recently completed the observations of L1451, and results for that region will be revealed at the meeting. Released CLASSy data products can be found on our project website.Fil: Storm, Shaye. University of Maryland; Estados UnidosFil: Mundy, Lee G.. University of Maryland; Estados UnidosFil: Teuben, Peter J.. University of Maryland; Estados UnidosFil: Lee, Katherine. University of Maryland; Estados UnidosFil: Looney, Leslie. University of Illinois at Urbana; 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: Rosolowsky, Erik. University of Alberta; CanadáFil: Arce, Hector G.. University of Yale; Estados UnidosFil: Shirley, Yancy L.. University of Arizona; Estados UnidosFil: Segura Cox, Dominique. University of Illinois; Estados UnidosFil: Isella, Andrea. Caltech; Estados UnidosFil: CLASSy Collaboration. No especifíca;223rd American Astronomical Society MeetingWashingtonEstados UnidosAmerican Astronomical SocietyAmerican Astronomical Society2014info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObjectCongresoJournalhttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/141612Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451; 223rd American Astronomical Society Meeting; Washington; Estados Unidos; 2014; 366-3670002-7537CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://aas.org/meetings/aas223info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/articulo/2015/3/18/ediciones_anteriores_baaaNacionalinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:32:03Zoai:ri.conicet.gov.ar:11336/141612instacron: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 10:32:04.051CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
title |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
spellingShingle |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 Storm, Shaye MOLECULAR CLOUDS |
title_short |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
title_full |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
title_fullStr |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
title_full_unstemmed |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
title_sort |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451 |
dc.creator.none.fl_str_mv |
Storm, Shaye Mundy, Lee G. Teuben, Peter J. Lee, Katherine Looney, Leslie Fernandez Lopez, Manuel Rosolowsky, Erik Arce, Hector G. Shirley, Yancy L. Segura Cox, Dominique Isella, Andrea CLASSy Collaboration |
author |
Storm, Shaye |
author_facet |
Storm, Shaye Mundy, Lee G. Teuben, Peter J. Lee, Katherine Looney, Leslie Fernandez Lopez, Manuel Rosolowsky, Erik Arce, Hector G. Shirley, Yancy L. Segura Cox, Dominique Isella, Andrea CLASSy Collaboration |
author_role |
author |
author2 |
Mundy, Lee G. Teuben, Peter J. Lee, Katherine Looney, Leslie Fernandez Lopez, Manuel Rosolowsky, Erik Arce, Hector G. Shirley, Yancy L. Segura Cox, Dominique Isella, Andrea CLASSy Collaboration |
author2_role |
author author author author author author author author author author author |
dc.subject.none.fl_str_mv |
MOLECULAR CLOUDS |
topic |
MOLECULAR CLOUDS |
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 spectral line maps of the dense gas across 400 square arcminutes of the Perseus Molecular Cloud, focused on NGC 1333, Barnard 1, and L1451. We constructed these maps as part of the CARMA Large Area Star-formation Survey (CLASSy), which is a CARMA key project that connects star forming cores to their natal cloud environment. This is achieved by leveraging CARMA's high angular resolution, imaging capability, and high efficiency at mosaicing large areas of the sky. CLASSy maps capture the structure and kinematics of N2H+, HCN, and HCO+ J=1-0 emission from thousand AU to parsec scales in three evolutionarily distinct regions of Perseus (in addition to two regions in Serpens). We show results from a non-binary dendrogram analysis of the Perseus N2H+ emission, which answers questions about the turbulent properties of the dense gas across evolutionary stages and across the range of size scales probed by CLASSy. There is a flat relation between mean internal turbulence and structure size for the dense gas in NGC 1333 and Barnard 1, but the magnitude of internal turbulence increases with nearby protostellar activity; the dense gas in the B1 main core and NGC 1333, which have active young stars, are characterized by mostly transonic to supersonic turbulence, while the filaments and clumps southwest of the B1 main core, which have no active young stars, have mostly subsonic turbulence. We have recently completed the observations of L1451, and results for that region will be revealed at the meeting. Released CLASSy data products can be found on our project website. Fil: Storm, Shaye. University of Maryland; Estados Unidos Fil: Mundy, Lee G.. University of Maryland; Estados Unidos Fil: Teuben, Peter J.. University of Maryland; Estados Unidos Fil: Lee, Katherine. University of Maryland; Estados Unidos Fil: Looney, Leslie. University of Illinois at Urbana; 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: Rosolowsky, Erik. University of Alberta; Canadá Fil: Arce, Hector G.. University of Yale; Estados Unidos Fil: Shirley, Yancy L.. University of Arizona; Estados Unidos Fil: Segura Cox, Dominique. University of Illinois; Estados Unidos Fil: Isella, Andrea. Caltech; Estados Unidos Fil: CLASSy Collaboration. No especifíca; 223rd American Astronomical Society Meeting Washington Estados Unidos American Astronomical Society |
description |
We present spectral line maps of the dense gas across 400 square arcminutes of the Perseus Molecular Cloud, focused on NGC 1333, Barnard 1, and L1451. We constructed these maps as part of the CARMA Large Area Star-formation Survey (CLASSy), which is a CARMA key project that connects star forming cores to their natal cloud environment. This is achieved by leveraging CARMA's high angular resolution, imaging capability, and high efficiency at mosaicing large areas of the sky. CLASSy maps capture the structure and kinematics of N2H+, HCN, and HCO+ J=1-0 emission from thousand AU to parsec scales in three evolutionarily distinct regions of Perseus (in addition to two regions in Serpens). We show results from a non-binary dendrogram analysis of the Perseus N2H+ emission, which answers questions about the turbulent properties of the dense gas across evolutionary stages and across the range of size scales probed by CLASSy. There is a flat relation between mean internal turbulence and structure size for the dense gas in NGC 1333 and Barnard 1, but the magnitude of internal turbulence increases with nearby protostellar activity; the dense gas in the B1 main core and NGC 1333, which have active young stars, are characterized by mostly transonic to supersonic turbulence, while the filaments and clumps southwest of the B1 main core, which have no active young stars, have mostly subsonic turbulence. We have recently completed the observations of L1451, and results for that region will be revealed at the meeting. Released CLASSy data products can be found on our project website. |
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 Congreso 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/11336/141612 Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451; 223rd American Astronomical Society Meeting; Washington; Estados Unidos; 2014; 366-367 0002-7537 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/141612 |
identifier_str_mv |
Dendrogram Analysis of Large-Area CARMA Images in Perseus: the Dense Gas in NGC 1333, Barnard 1, and L1451; 223rd American Astronomical Society Meeting; Washington; Estados Unidos; 2014; 366-367 0002-7537 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/meetings/aas223 info:eu-repo/semantics/altIdentifier/url/http://www.astronomiaargentina.org.ar/articulo/2015/3/18/ediciones_anteriores_baaa |
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 |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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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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