Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1

Autores
Storm, Shaye; Mundy, Lee G.; Fernandez Lopez, Manuel; Lee, Katherine I.; Looney, Leslie W.; Teuben, Peter; Rosolowsky, Erik W.; Arce, Héctor G.; Ostriker, Eve C.; Segura-Cox, Dominique M.; Pound, Marc W.; Salter, Demerese M.; Volgenau, Nikolaus H.; Shirley, Yancy L.; Chen, Che Yu; Gong, Hao; Plunkett, Adele L.; Tobin, John J.; Kwon, Woojin; Isella, Andrea; Kauffmann, Jens; Tassis, Konstantinos; Crutcher, Richard M.; Gammie, Charles F.; Testi, Leonardo
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J = 1 → 0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7'' and spectral resolution near 0.16 km s–1. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N2H+ shows the strongest emission, with morphology similar to cool dust in the region, while HCO+ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N2H+ velocity dispersions ranging from ~0.05 to 0.50 km s–1 across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new, non-binary dendrogram algorithm is used to analyze dense gas structures in the N2H+ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01 to 0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc this suggests that overdense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download.
Fil: Storm, Shaye . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Mundy, Lee G. . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Fernandez Lopez, Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Lee, Katherine I. . University of Maryland. Department of Astronomy;; Estados Unidos
Fil: Looney, Leslie W. . University of Illinois, Urbana Department of Astronomy; Estados Unidos
Fil: Teuben, Peter . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Rosolowsky, Erik W. . University of British Columbia. Departments of Physics and Statistics; Canadá
Fil: Arce, Héctor G. . Yale University. Department of Astronomy; Estados Unidos
Fil: Ostriker, Eve C. . Princeton University. Department of Astrophysical Sciences; Estados Unidos
Fil: Segura-Cox, Dominique M.. University of Illinois, Urbana. Department of Astronomy; Estados Unidos
Fil: Pound, Marc W. . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Salter, Demerese M. . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Volgenau, Nikolaus H. . Owens Valley Radio Observatory; Estados Unidos
Fil: Shirley, Yancy L. . Steward Observatory, Tucson; Estados Unidos
Fil: Chen, Che Yu . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Gong, Hao . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Plunkett, Adele L. . Yale University. Department of Astronomy; Estados Unidos
Fil: Tobin, John J. . National Radio Astronomy Observatory; Estados Unidos
Fil: Kwon, Woojin . SRON Netherlands Institute for Space Research; Países Bajos
Fil: Isella, Andrea . California Institute of Technology. Astronomy Department; Estados Unidos
Fil: Kauffmann, Jens . Max Planck Institut für Radioastronomie; Alemania
Fil: Tassis, Konstantinos . University of Crete. Department of Physics and Institute of Theoretical and Computational Physics; Grecia
Fil: Crutcher, Richard M. . University of Illinois, Urbana. Department of Astronomy; Estados Unidos
Fil: Gammie, Charles F. . University of Illinois, Urbana. Department of Astronomy; Estados Unidos
Fil: Testi, Leonardo . ESO, Karl-Schwarzschild-Strasse; Alemania
Materia
Barnard 1
Interstellar Medium
Turbulence
CLASSy
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:11336/7276

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network_name_str CONICET Digital (CONICET)
spelling Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1Storm, Shaye Mundy, Lee G. Fernandez Lopez, ManuelLee, Katherine I. Looney, Leslie W. Teuben, Peter Rosolowsky, Erik W. Arce, Héctor G. Ostriker, Eve C. Segura-Cox, Dominique M.Pound, Marc W. Salter, Demerese M. Volgenau, Nikolaus H. Shirley, Yancy L. Chen, Che Yu Gong, Hao Plunkett, Adele L. Tobin, John J. Kwon, Woojin Isella, Andrea Kauffmann, Jens Tassis, Konstantinos Crutcher, Richard M. Gammie, Charles F. Testi, Leonardo Barnard 1Interstellar MediumTurbulenceCLASSyhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J = 1 → 0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7'' and spectral resolution near 0.16 km s–1. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N2H+ shows the strongest emission, with morphology similar to cool dust in the region, while HCO+ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N2H+ velocity dispersions ranging from ~0.05 to 0.50 km s–1 across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new, non-binary dendrogram algorithm is used to analyze dense gas structures in the N2H+ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01 to 0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc this suggests that overdense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download.Fil: Storm, Shaye . University of Maryland. Department of Astronomy; Estados UnidosFil: Mundy, Lee G. . University of Maryland. Department of Astronomy; Estados UnidosFil: Fernandez Lopez, Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); ArgentinaFil: Lee, Katherine I. . University of Maryland. Department of Astronomy;; Estados UnidosFil: Looney, Leslie W. . University of Illinois, Urbana Department of Astronomy; Estados UnidosFil: Teuben, Peter . University of Maryland. Department of Astronomy; Estados UnidosFil: Rosolowsky, Erik W. . University of British Columbia. Departments of Physics and Statistics; CanadáFil: Arce, Héctor G. . Yale University. Department of Astronomy; Estados UnidosFil: Ostriker, Eve C. . Princeton University. Department of Astrophysical Sciences; Estados UnidosFil: Segura-Cox, Dominique M.. University of Illinois, Urbana. Department of Astronomy; Estados UnidosFil: Pound, Marc W. . University of Maryland. Department of Astronomy; Estados UnidosFil: Salter, Demerese M. . University of Maryland. Department of Astronomy; Estados UnidosFil: Volgenau, Nikolaus H. . Owens Valley Radio Observatory; Estados UnidosFil: Shirley, Yancy L. . Steward Observatory, Tucson; Estados UnidosFil: Chen, Che Yu . University of Maryland. Department of Astronomy; Estados UnidosFil: Gong, Hao . University of Maryland. Department of Astronomy; Estados UnidosFil: Plunkett, Adele L. . Yale University. Department of Astronomy; Estados UnidosFil: Tobin, John J. . National Radio Astronomy Observatory; Estados UnidosFil: Kwon, Woojin . SRON Netherlands Institute for Space Research; Países BajosFil: Isella, Andrea . California Institute of Technology. Astronomy Department; Estados UnidosFil: Kauffmann, Jens . Max Planck Institut für Radioastronomie; AlemaniaFil: Tassis, Konstantinos . University of Crete. Department of Physics and Institute of Theoretical and Computational Physics; GreciaFil: Crutcher, Richard M. . University of Illinois, Urbana. Department of Astronomy; Estados UnidosFil: Gammie, Charles F. . University of Illinois, Urbana. Department of Astronomy; Estados UnidosFil: Testi, Leonardo . ESO, Karl-Schwarzschild-Strasse; AlemaniaIOP Publishing2014-10info: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/11336/7276Storm, Shaye ; Mundy, Lee G. ; Fernandez Lopez, Manuel; Lee, Katherine I. ; Looney, Leslie W. ; et al.; Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1; IOP Publishing; Astrophysical Journal; 794; 2; 10-2014; 165-1650004-637Xenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/794/2/165/metainfo:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1409.1233info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/794/2/165info:eu-repo/semantics/altIdentifier/doi/info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:08:47Zoai:ri.conicet.gov.ar:11336/7276instacron: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 10:08:47.309CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
title Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
spellingShingle Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
Storm, Shaye
Barnard 1
Interstellar Medium
Turbulence
CLASSy
title_short Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
title_full Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
title_fullStr Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
title_full_unstemmed Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
title_sort Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1
dc.creator.none.fl_str_mv Storm, Shaye
Mundy, Lee G.
Fernandez Lopez, Manuel
Lee, Katherine I.
Looney, Leslie W.
Teuben, Peter
Rosolowsky, Erik W.
Arce, Héctor G.
Ostriker, Eve C.
Segura-Cox, Dominique M.
Pound, Marc W.
Salter, Demerese M.
Volgenau, Nikolaus H.
Shirley, Yancy L.
Chen, Che Yu
Gong, Hao
Plunkett, Adele L.
Tobin, John J.
Kwon, Woojin
Isella, Andrea
Kauffmann, Jens
Tassis, Konstantinos
Crutcher, Richard M.
Gammie, Charles F.
Testi, Leonardo
author Storm, Shaye
author_facet Storm, Shaye
Mundy, Lee G.
Fernandez Lopez, Manuel
Lee, Katherine I.
Looney, Leslie W.
Teuben, Peter
Rosolowsky, Erik W.
Arce, Héctor G.
Ostriker, Eve C.
Segura-Cox, Dominique M.
Pound, Marc W.
Salter, Demerese M.
Volgenau, Nikolaus H.
Shirley, Yancy L.
Chen, Che Yu
Gong, Hao
Plunkett, Adele L.
Tobin, John J.
Kwon, Woojin
Isella, Andrea
Kauffmann, Jens
Tassis, Konstantinos
Crutcher, Richard M.
Gammie, Charles F.
Testi, Leonardo
author_role author
author2 Mundy, Lee G.
Fernandez Lopez, Manuel
Lee, Katherine I.
Looney, Leslie W.
Teuben, Peter
Rosolowsky, Erik W.
Arce, Héctor G.
Ostriker, Eve C.
Segura-Cox, Dominique M.
Pound, Marc W.
Salter, Demerese M.
Volgenau, Nikolaus H.
Shirley, Yancy L.
Chen, Che Yu
Gong, Hao
Plunkett, Adele L.
Tobin, John J.
Kwon, Woojin
Isella, Andrea
Kauffmann, Jens
Tassis, Konstantinos
Crutcher, Richard M.
Gammie, Charles F.
Testi, Leonardo
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv Barnard 1
Interstellar Medium
Turbulence
CLASSy
topic Barnard 1
Interstellar Medium
Turbulence
CLASSy
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 details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J = 1 → 0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7'' and spectral resolution near 0.16 km s–1. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N2H+ shows the strongest emission, with morphology similar to cool dust in the region, while HCO+ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N2H+ velocity dispersions ranging from ~0.05 to 0.50 km s–1 across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new, non-binary dendrogram algorithm is used to analyze dense gas structures in the N2H+ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01 to 0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc this suggests that overdense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download.
Fil: Storm, Shaye . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Mundy, Lee G. . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Fernandez Lopez, Manuel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico la Plata. Instituto Argentino de Radioastronomia (i); Argentina
Fil: Lee, Katherine I. . University of Maryland. Department of Astronomy;; Estados Unidos
Fil: Looney, Leslie W. . University of Illinois, Urbana Department of Astronomy; Estados Unidos
Fil: Teuben, Peter . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Rosolowsky, Erik W. . University of British Columbia. Departments of Physics and Statistics; Canadá
Fil: Arce, Héctor G. . Yale University. Department of Astronomy; Estados Unidos
Fil: Ostriker, Eve C. . Princeton University. Department of Astrophysical Sciences; Estados Unidos
Fil: Segura-Cox, Dominique M.. University of Illinois, Urbana. Department of Astronomy; Estados Unidos
Fil: Pound, Marc W. . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Salter, Demerese M. . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Volgenau, Nikolaus H. . Owens Valley Radio Observatory; Estados Unidos
Fil: Shirley, Yancy L. . Steward Observatory, Tucson; Estados Unidos
Fil: Chen, Che Yu . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Gong, Hao . University of Maryland. Department of Astronomy; Estados Unidos
Fil: Plunkett, Adele L. . Yale University. Department of Astronomy; Estados Unidos
Fil: Tobin, John J. . National Radio Astronomy Observatory; Estados Unidos
Fil: Kwon, Woojin . SRON Netherlands Institute for Space Research; Países Bajos
Fil: Isella, Andrea . California Institute of Technology. Astronomy Department; Estados Unidos
Fil: Kauffmann, Jens . Max Planck Institut für Radioastronomie; Alemania
Fil: Tassis, Konstantinos . University of Crete. Department of Physics and Institute of Theoretical and Computational Physics; Grecia
Fil: Crutcher, Richard M. . University of Illinois, Urbana. Department of Astronomy; Estados Unidos
Fil: Gammie, Charles F. . University of Illinois, Urbana. Department of Astronomy; Estados Unidos
Fil: Testi, Leonardo . ESO, Karl-Schwarzschild-Strasse; Alemania
description We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N2H+, HCO+, and HCN (J = 1 → 0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7'' and spectral resolution near 0.16 km s–1. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N2H+ shows the strongest emission, with morphology similar to cool dust in the region, while HCO+ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N2H+ velocity dispersions ranging from ~0.05 to 0.50 km s–1 across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new, non-binary dendrogram algorithm is used to analyze dense gas structures in the N2H+ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01 to 0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc this suggests that overdense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download.
publishDate 2014
dc.date.none.fl_str_mv 2014-10
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/11336/7276
Storm, Shaye ; Mundy, Lee G. ; Fernandez Lopez, Manuel; Lee, Katherine I. ; Looney, Leslie W. ; et al.; Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1; IOP Publishing; Astrophysical Journal; 794; 2; 10-2014; 165-165
0004-637X
url http://hdl.handle.net/11336/7276
identifier_str_mv Storm, Shaye ; Mundy, Lee G. ; Fernandez Lopez, Manuel; Lee, Katherine I. ; Looney, Leslie W. ; et al.; Carma Large Area Star Formation Survey: project overview with analysis of dense gas structure and kinematics in barnard 1; IOP Publishing; Astrophysical Journal; 794; 2; 10-2014; 165-165
0004-637X
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.1088/0004-637X/794/2/165/meta
info:eu-repo/semantics/altIdentifier/arxiv/http://arxiv.org/abs/1409.1233
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/794/2/165
info:eu-repo/semantics/altIdentifier/doi/
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 IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
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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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