Carma large area star formation survey : dense gas in the young L1451 region of Perseus
- Autores
- Storm, Shaye; Mundy, Lee G.; Lee, Katherine I.; Fernandez Lopez, Manuel; Looney, Leslie W.; Teuben, Peter; Arce, Héctor G.; Rosolowsky, Erik W.; Meisner, Aaron M.; Isella, Andrea; Kauffmann, Jens; Shirley, Yancy L.; Kwon, Woojin; Plunkett, Adele L.; Pound, Marc W.; Segura Cox, Dominique M.; Tassis, Konstantinos; Tobin, John J.; Volgenau, Nikolaus H.; Crutcher, Richard M.; Testi, Leonardo
- Año de publicación
- 2016
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We present a 3 mm spectral line and continuum survey of L1451 in the Perseus Molecular Cloud. These observations are from the CARMA Large Area Star Formation Survey (CLASSy), which also imaged Barnard 1, NGC 1333, Serpens Main, and Serpens South. L1451 is the survey region with the lowest level of star formation activity - it contains no confirmed protostars. HCO+, HCN, and N2H+ are all detected throughout the region, with HCO+ being the most spatially widespread, and molecular emission seen toward 90% of the area above N(H2) column densities of 1.9 1021 cm-2. HCO+ has the broadest velocity dispersion, near 0.3 km s-1 on average, compared with ∼0.15 km s-1 for the other molecules, thus representing a range of subsonic to supersonic gas motions. Our non-binary dendrogram analysis reveals that the dense gas traced by each molecule has a similar hierarchical structure, and that gas surrounding the candidate first hydrostatic core (FHSC), L1451-mm, and other previously detected single-dish continuum clumps has similar hierarchical structure; this suggests that different subregions of L1451 are fragmenting on the pathway to forming young stars. We determined that the three-dimensional morphology of the largest detectable dense-gas structures was relatively ellipsoidal compared with other CLASSy regions, which appeared more flattened at the largest scales. A virial analysis shows that the most centrally condensed dust structures are likely unstable against collapse. Additionally, we identify a new spherical, centrally condensed N2H+ feature that could be a new FHSC candidate. The overall results suggest that L1451 is a young region starting to form its generation of stars within turbulent, hierarchical structures.
Fil: Storm, Shaye. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Maryland; Estados Unidos
Fil: Mundy, Lee G.. University of Maryland; Estados Unidos
Fil: Lee, Katherine I.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Maryland; Estados Unidos
Fil: Fernandez Lopez, Manuel. University Of Illinois. Urbana - Champaign; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina
Fil: Looney, Leslie W.. University Of Illinois. Urbana - Champaign; Estados Unidos
Fil: Teuben, Peter. University of Maryland; Estados Unidos
Fil: Arce, Héctor G.. University of Yale; Estados Unidos
Fil: Rosolowsky, Erik W.. University of Alberta; Canadá
Fil: Meisner, Aaron M.. Lawrence Berkeley National Laboratory; Estados Unidos
Fil: Isella, Andrea. Rice University; Estados Unidos
Fil: Kauffmann, Jens. Max Planck Institut Fur Radioastronomie; Alemania
Fil: Shirley, Yancy L.. University of Arizona; Estados Unidos
Fil: Kwon, Woojin. Korea Astronomy And Space Science Institute; Corea del Sur
Fil: Plunkett, Adele L.. European Southern Observatory; Chile
Fil: Pound, Marc W.. University of Maryland; Estados Unidos
Fil: Segura Cox, Dominique M.. University Of Illinois. Urbana - Champaign; Estados Unidos
Fil: Tassis, Konstantinos. Foundation For Research And Technology; Grecia
Fil: Tobin, John J.. Leiden Observatory Research Institute; Países Bajos
Fil: Volgenau, Nikolaus H.. Las Cumbres Observatory Global Telescope Network; Estados Unidos
Fil: Crutcher, Richard M.. University Of Illinois. Urbana - Champaign; Estados Unidos
Fil: Testi, Leonardo. European Southern Observatory; Chile - Materia
-
Clouds
Kinematics and dynamics
Molecules
Machine readeable tables
Star formation - 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:11336/27399
Ver los metadatos del registro completo
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Carma large area star formation survey : dense gas in the young L1451 region of PerseusStorm, ShayeMundy, Lee G.Lee, Katherine I.Fernandez Lopez, ManuelLooney, Leslie W.Teuben, PeterArce, Héctor G.Rosolowsky, Erik W.Meisner, Aaron M.Isella, AndreaKauffmann, JensShirley, Yancy L.Kwon, WoojinPlunkett, Adele L.Pound, Marc W.Segura Cox, Dominique M.Tassis, KonstantinosTobin, John J.Volgenau, Nikolaus H.Crutcher, Richard M.Testi, LeonardoCloudsKinematics and dynamicsMoleculesMachine readeable tablesStar formationhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a 3 mm spectral line and continuum survey of L1451 in the Perseus Molecular Cloud. These observations are from the CARMA Large Area Star Formation Survey (CLASSy), which also imaged Barnard 1, NGC 1333, Serpens Main, and Serpens South. L1451 is the survey region with the lowest level of star formation activity - it contains no confirmed protostars. HCO+, HCN, and N2H+ are all detected throughout the region, with HCO+ being the most spatially widespread, and molecular emission seen toward 90% of the area above N(H2) column densities of 1.9 1021 cm-2. HCO+ has the broadest velocity dispersion, near 0.3 km s-1 on average, compared with ∼0.15 km s-1 for the other molecules, thus representing a range of subsonic to supersonic gas motions. Our non-binary dendrogram analysis reveals that the dense gas traced by each molecule has a similar hierarchical structure, and that gas surrounding the candidate first hydrostatic core (FHSC), L1451-mm, and other previously detected single-dish continuum clumps has similar hierarchical structure; this suggests that different subregions of L1451 are fragmenting on the pathway to forming young stars. We determined that the three-dimensional morphology of the largest detectable dense-gas structures was relatively ellipsoidal compared with other CLASSy regions, which appeared more flattened at the largest scales. A virial analysis shows that the most centrally condensed dust structures are likely unstable against collapse. Additionally, we identify a new spherical, centrally condensed N2H+ feature that could be a new FHSC candidate. The overall results suggest that L1451 is a young region starting to form its generation of stars within turbulent, hierarchical structures.Fil: Storm, Shaye. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Maryland; Estados UnidosFil: Mundy, Lee G.. University of Maryland; Estados UnidosFil: Lee, Katherine I.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Maryland; Estados UnidosFil: Fernandez Lopez, Manuel. University Of Illinois. Urbana - Champaign; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; ArgentinaFil: Looney, Leslie W.. University Of Illinois. Urbana - Champaign; Estados UnidosFil: Teuben, Peter. University of Maryland; Estados UnidosFil: Arce, Héctor G.. University of Yale; Estados UnidosFil: Rosolowsky, Erik W.. University of Alberta; CanadáFil: Meisner, Aaron M.. Lawrence Berkeley National Laboratory; Estados UnidosFil: Isella, Andrea. Rice University; Estados UnidosFil: Kauffmann, Jens. Max Planck Institut Fur Radioastronomie; AlemaniaFil: Shirley, Yancy L.. University of Arizona; Estados UnidosFil: Kwon, Woojin. Korea Astronomy And Space Science Institute; Corea del SurFil: Plunkett, Adele L.. European Southern Observatory; ChileFil: Pound, Marc W.. University of Maryland; Estados UnidosFil: Segura Cox, Dominique M.. University Of Illinois. Urbana - Champaign; Estados UnidosFil: Tassis, Konstantinos. Foundation For Research And Technology; GreciaFil: Tobin, John J.. Leiden Observatory Research Institute; Países BajosFil: Volgenau, Nikolaus H.. Las Cumbres Observatory Global Telescope Network; Estados UnidosFil: Crutcher, Richard M.. University Of Illinois. Urbana - Champaign; Estados UnidosFil: Testi, Leonardo. European Southern Observatory; ChileIOP Publishing2016-10info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/27399Storm, Shaye; Mundy, Lee G.; Lee, Katherine I.; Fernandez Lopez, Manuel; Looney, Leslie W.; et al.; Carma large area star formation survey : dense gas in the young L1451 region of Perseus; IOP Publishing; Astrophysical Journal; 830; 2; 10-2016; 1-450004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/830/2/127info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0004-637X/830/2/127/metainfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:35:12Zoai:ri.conicet.gov.ar:11336/27399instacron: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 09:35:12.401CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
title |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
spellingShingle |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus Storm, Shaye Clouds Kinematics and dynamics Molecules Machine readeable tables Star formation |
title_short |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
title_full |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
title_fullStr |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
title_full_unstemmed |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
title_sort |
Carma large area star formation survey : dense gas in the young L1451 region of Perseus |
dc.creator.none.fl_str_mv |
Storm, Shaye Mundy, Lee G. Lee, Katherine I. Fernandez Lopez, Manuel Looney, Leslie W. Teuben, Peter Arce, Héctor G. Rosolowsky, Erik W. Meisner, Aaron M. Isella, Andrea Kauffmann, Jens Shirley, Yancy L. Kwon, Woojin Plunkett, Adele L. Pound, Marc W. Segura Cox, Dominique M. Tassis, Konstantinos Tobin, John J. Volgenau, Nikolaus H. Crutcher, Richard M. Testi, Leonardo |
author |
Storm, Shaye |
author_facet |
Storm, Shaye Mundy, Lee G. Lee, Katherine I. Fernandez Lopez, Manuel Looney, Leslie W. Teuben, Peter Arce, Héctor G. Rosolowsky, Erik W. Meisner, Aaron M. Isella, Andrea Kauffmann, Jens Shirley, Yancy L. Kwon, Woojin Plunkett, Adele L. Pound, Marc W. Segura Cox, Dominique M. Tassis, Konstantinos Tobin, John J. Volgenau, Nikolaus H. Crutcher, Richard M. Testi, Leonardo |
author_role |
author |
author2 |
Mundy, Lee G. Lee, Katherine I. Fernandez Lopez, Manuel Looney, Leslie W. Teuben, Peter Arce, Héctor G. Rosolowsky, Erik W. Meisner, Aaron M. Isella, Andrea Kauffmann, Jens Shirley, Yancy L. Kwon, Woojin Plunkett, Adele L. Pound, Marc W. Segura Cox, Dominique M. Tassis, Konstantinos Tobin, John J. Volgenau, Nikolaus H. Crutcher, Richard M. Testi, Leonardo |
author2_role |
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 |
Clouds Kinematics and dynamics Molecules Machine readeable tables Star formation |
topic |
Clouds Kinematics and dynamics Molecules Machine readeable tables 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 3 mm spectral line and continuum survey of L1451 in the Perseus Molecular Cloud. These observations are from the CARMA Large Area Star Formation Survey (CLASSy), which also imaged Barnard 1, NGC 1333, Serpens Main, and Serpens South. L1451 is the survey region with the lowest level of star formation activity - it contains no confirmed protostars. HCO+, HCN, and N2H+ are all detected throughout the region, with HCO+ being the most spatially widespread, and molecular emission seen toward 90% of the area above N(H2) column densities of 1.9 1021 cm-2. HCO+ has the broadest velocity dispersion, near 0.3 km s-1 on average, compared with ∼0.15 km s-1 for the other molecules, thus representing a range of subsonic to supersonic gas motions. Our non-binary dendrogram analysis reveals that the dense gas traced by each molecule has a similar hierarchical structure, and that gas surrounding the candidate first hydrostatic core (FHSC), L1451-mm, and other previously detected single-dish continuum clumps has similar hierarchical structure; this suggests that different subregions of L1451 are fragmenting on the pathway to forming young stars. We determined that the three-dimensional morphology of the largest detectable dense-gas structures was relatively ellipsoidal compared with other CLASSy regions, which appeared more flattened at the largest scales. A virial analysis shows that the most centrally condensed dust structures are likely unstable against collapse. Additionally, we identify a new spherical, centrally condensed N2H+ feature that could be a new FHSC candidate. The overall results suggest that L1451 is a young region starting to form its generation of stars within turbulent, hierarchical structures. Fil: Storm, Shaye. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Maryland; Estados Unidos Fil: Mundy, Lee G.. University of Maryland; Estados Unidos Fil: Lee, Katherine I.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos. University of Maryland; Estados Unidos Fil: Fernandez Lopez, Manuel. University Of Illinois. Urbana - Champaign; Estados Unidos. Provincia de Buenos Aires. Gobernación. Comision de Investigaciones Científicas. Instituto Argentino de Radioastronomía. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto Argentino de Radioastronomia; Argentina Fil: Looney, Leslie W.. University Of Illinois. Urbana - Champaign; Estados Unidos Fil: Teuben, Peter. University of Maryland; Estados Unidos Fil: Arce, Héctor G.. University of Yale; Estados Unidos Fil: Rosolowsky, Erik W.. University of Alberta; Canadá Fil: Meisner, Aaron M.. Lawrence Berkeley National Laboratory; Estados Unidos Fil: Isella, Andrea. Rice University; Estados Unidos Fil: Kauffmann, Jens. Max Planck Institut Fur Radioastronomie; Alemania Fil: Shirley, Yancy L.. University of Arizona; Estados Unidos Fil: Kwon, Woojin. Korea Astronomy And Space Science Institute; Corea del Sur Fil: Plunkett, Adele L.. European Southern Observatory; Chile Fil: Pound, Marc W.. University of Maryland; Estados Unidos Fil: Segura Cox, Dominique M.. University Of Illinois. Urbana - Champaign; Estados Unidos Fil: Tassis, Konstantinos. Foundation For Research And Technology; Grecia Fil: Tobin, John J.. Leiden Observatory Research Institute; Países Bajos Fil: Volgenau, Nikolaus H.. Las Cumbres Observatory Global Telescope Network; Estados Unidos Fil: Crutcher, Richard M.. University Of Illinois. Urbana - Champaign; Estados Unidos Fil: Testi, Leonardo. European Southern Observatory; Chile |
description |
We present a 3 mm spectral line and continuum survey of L1451 in the Perseus Molecular Cloud. These observations are from the CARMA Large Area Star Formation Survey (CLASSy), which also imaged Barnard 1, NGC 1333, Serpens Main, and Serpens South. L1451 is the survey region with the lowest level of star formation activity - it contains no confirmed protostars. HCO+, HCN, and N2H+ are all detected throughout the region, with HCO+ being the most spatially widespread, and molecular emission seen toward 90% of the area above N(H2) column densities of 1.9 1021 cm-2. HCO+ has the broadest velocity dispersion, near 0.3 km s-1 on average, compared with ∼0.15 km s-1 for the other molecules, thus representing a range of subsonic to supersonic gas motions. Our non-binary dendrogram analysis reveals that the dense gas traced by each molecule has a similar hierarchical structure, and that gas surrounding the candidate first hydrostatic core (FHSC), L1451-mm, and other previously detected single-dish continuum clumps has similar hierarchical structure; this suggests that different subregions of L1451 are fragmenting on the pathway to forming young stars. We determined that the three-dimensional morphology of the largest detectable dense-gas structures was relatively ellipsoidal compared with other CLASSy regions, which appeared more flattened at the largest scales. A virial analysis shows that the most centrally condensed dust structures are likely unstable against collapse. Additionally, we identify a new spherical, centrally condensed N2H+ feature that could be a new FHSC candidate. The overall results suggest that L1451 is a young region starting to form its generation of stars within turbulent, hierarchical structures. |
publishDate |
2016 |
dc.date.none.fl_str_mv |
2016-10 |
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/11336/27399 Storm, Shaye; Mundy, Lee G.; Lee, Katherine I.; Fernandez Lopez, Manuel; Looney, Leslie W.; et al.; Carma large area star formation survey : dense gas in the young L1451 region of Perseus; IOP Publishing; Astrophysical Journal; 830; 2; 10-2016; 1-45 0004-637X CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/27399 |
identifier_str_mv |
Storm, Shaye; Mundy, Lee G.; Lee, Katherine I.; Fernandez Lopez, Manuel; Looney, Leslie W.; et al.; Carma large area star formation survey : dense gas in the young L1451 region of Perseus; IOP Publishing; Astrophysical Journal; 830; 2; 10-2016; 1-45 0004-637X CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.3847/0004-637X/830/2/127 info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/article/10.3847/0004-637X/830/2/127/meta |
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.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 |
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1844613094481854464 |
score |
13.070432 |