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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/7276
Ver los metadatos del registro completo
id |
CONICETDig_a4947b8d7f5ec287be1f4e4f5b1453d1 |
---|---|
oai_identifier_str |
oai:ri.conicet.gov.ar:11336/7276 |
network_acronym_str |
CONICETDig |
repository_id_str |
3498 |
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) |
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 |
_version_ |
1844613958630113280 |
score |
13.070432 |