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Core fragmentation and Toomre stability analysis of W3(H<sub>2</sub>O) A case study of the IRAM NOEMA large program CORE
| Indexado |
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| DOI | 10.1051/0004-6361/201732548 | ||||
| Año | 2018 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Abstract
Conclusions. Combining millimetre dust continuum and spectral line data toward the famous high-mass star-forming region W3(H2O), we identify core fragmentation on large scales, and indications for possible disk fragmentation on smaller spatial scales.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Ahmadi, A. | - |
Max Planck Inst Astron - Alemania
Heidelberg Univ - Alemania Max Planck Institute for Astronomy - Alemania Universität Heidelberg - Alemania International Max Planck Research School for Astronomy & Cosmic Physics at the University of Heidelberg - Alemania |
| 2 | Beuther, H. | Hombre |
Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania |
| 3 | Mottram, J. C. | Hombre |
Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania |
| 4 | Bosco, F. | - |
Max Planck Inst Astron - Alemania
Heidelberg Univ - Alemania Max Planck Institute for Astronomy - Alemania Universität Heidelberg - Alemania International Max Planck Research School for Astronomy & Cosmic Physics at the University of Heidelberg - Alemania |
| 5 | Linz, Hendrik | Hombre |
Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania |
| 6 | Henning, Thomas | Hombre |
Max Planck Inst Astron - Alemania
Max Planck Institute for Astronomy - Alemania |
| 7 | Winters, J. M. | Hombre |
IRAM - Francia
Universite Grenoble Alpes - Francia |
| 8 | Kuiper, R. | Hombre |
UNIV TUBINGEN - Alemania
Universität Tübingen - Alemania Eberhard Karls Universität Tübingen - Alemania |
| 9 | Pudritz, R. | - |
MCMASTER UNIV - Canadá
McMaster University, Faculty of Science - Canadá McMaster University - Canadá |
| 10 | Sanchez-Monge, Alvaro | Hombre |
Univ Cologne - Alemania
University of Cologne - Alemania Universität zu Köln - Alemania |
| 11 | Keto, E. R. | Hombre |
Harvard Smithsonian Ctr Astrophys - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos |
| 12 | Beltran, Maria T. | Mujer |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astrofisico Di Arcetri - Italia INAF - Italia |
| 13 | Bontemps, S. | Hombre |
Univ Bordeaux 1 - Francia
Laboratoire d'Astrophysique de Bordeaux - Francia |
| 14 | Cesaroni, R. | Mujer |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astrofisico Di Arcetri - Italia INAF - Italia |
| 15 | Csengeri, T. | - |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania Max Planck Inst Astron - Alemania |
| 16 | Feng, S. | - |
Max Planck Inst Extraterr Phys - Alemania
Max Planck Institute for Extraterrestrial Physics - Alemania |
| 17 | GARAY BRIGNARDELLO, GUIDO ALEJANDRO | Hombre |
Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México Instituto de Radioastronomía y Astrofísica - México |
| 18 | Johnston, Katharine G. | Mujer |
UNIV LEEDS - Reino Unido
University of Leeds - Reino Unido |
| 19 | Klaassen, Pamela D. | Mujer |
Royal Observ Edinburgh - Reino Unido
Royal Observatory - Reino Unido |
| 20 | Leurini, S. | Mujer |
INAF Osservatorio Astron Cagliari - Italia
Osservatorio Astronomico di Cagliari - Italia |
| 21 | Longmore, S. N. | Hombre |
Liverpool John Moores Univ - Reino Unido
Liverpool John Moores University - Reino Unido |
| 22 | Lumsden, S. | - |
UNIV LEEDS - Reino Unido
University of Leeds - Reino Unido |
| 23 | Maud, Luke T. | Hombre |
Leiden Univ - Países Bajos
Leiden Observatory Research Institute - Países Bajos Sterrewacht Leiden - Países Bajos |
| 24 | Menten, K. M. | Hombre |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania Max Planck Inst Astron - Alemania |
| 25 | Moscadelli, L. | - |
Istituto Nazionale di Astrofisica - Italia
Osservatorio Astrofisico Di Arcetri - Italia INAF - Italia |
| 26 | Motte, F. | Mujer |
Univ Grenoble Alpes - Francia
Universite Grenoble Alpes - Francia |
| 27 | Palau, Aina | Mujer |
Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México Instituto de Radioastronomía y Astrofísica - México |
| 28 | Peters, T. | - |
Max Planck Inst Astrophys - Alemania
Max Planck Institute for Astrophysics - Alemania Max Planck Inst Astron - Alemania |
| 29 | Ragan, S. | Mujer |
Cardiff Univ - Reino Unido
Cardiff University - Reino Unido |
| 30 | Schilke, Peter | Hombre |
Univ Cologne - Alemania
University of Cologne - Alemania Universität zu Köln - Alemania |
| 31 | Urquhart, James | Hombre |
Univ Kent - Reino Unido
University of Kent - Reino Unido |
| 32 | MORA-FERNANDEZ, ALCIONE | Hombre |
Max Planck Inst Radioastron - Alemania
Max Planck Institute for Radio Astronomy - Alemania Max Planck Inst Astron - Alemania |
| 33 | Zinnecker, H. | Hombre |
NASA - Estados Unidos
Universidad Autónoma de Chile - Chile NASA Ames Research Center - Estados Unidos |
| Fuente |
|---|
| Consejo Nacional de Ciencia y Tecnología |
| Universidad Nacional Autónoma de México |
| Deutsche Forschungsgemeinschaft |
| European Research Council |
| STFC |
| UNAM, Mexico |
| CONACyT, Mexico |
| Centre National de la Recherche Scientifique |
| Horizon 2020 Framework Programme |
| Emmy Noether Research Group on Accretion Flows and Feedback in Realistic Models of Massive Star Formation - German Research Foundation (DFG) |
| INSU |
| Consejo Nacional de Ciencia y TecnologÃa, Paraguay |
| Deutsche For-schungsgemeinschaft |
| IIlinois State Museum |
| European Research Council under the European Community's Horizon 2020 framework programme (2014-2020) via the ERC Consolidator grant "From Cloud to Star Formation (CSF)" |
| Deutsche Forschungsgemeinschaft, DFG via the SPP (priority programme) "Physics of the ISM" |
| University of Namibia |
| European Community’s Horizon 2020 framework programme |
| Agradecimiento |
|---|
| The authors would like to thank the anonymous referee whose comments helped the clarity of this paper. We also thank Thomas Moller for his technical support with the XCLASS analysis, and Kaitlin Kratter for fruitful discussions regarding the Toomre Q stability analysis. A.A., H.B., J.C.M., and F.B. acknowledge support from the European Research Council under the European Community's Horizon 2020 framework programme (2014-2020) via the ERC Consolidator Grant "From Cloud to Star Formation (CSF)" (project number 648505). R.K. acknowledges financial support via the Emmy Noether Research Group on Accretion Flows and Feedback in Realistic Models of Massive Star Formation funded by the German Research Foundation (DFG) under grant no. KU 2849/3-1. T.Cs. acknowledges support from the Deutsche Forschungsgemeinschaft, DFG via the SPP (priority programme) 1573 "Physics of the ISM". A.P. acknowledges financial support from UNAM and CONACyT, Mexico. |
| ★Based on observations from an IRAM large program. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). |
