Molecular cloud evolution ― IV. Magnetic fields, ambipolar diffusion and the star formation efficiency
- Author
- VAZQUEZ-SEMADENI, Enrique1 ; BANERJEE, Robi2 ; GOMEZ, Gilberto C1 ; HENNEBELLE, Patrick3 ; DUFFIN, Dennis4 ; KLESSEN, Ralf S2
[1] Centro de Radioastronomia y Astrofísica, Universidad Nacional Autónoma de México, Campus Morelia, Apdo. Postal 3-72, Morelia 58089, Mexico
[2] Zentrum für Astronomie der Universität Heidelberg, Institut für Theoretische Astrophysik, 69120 Heidelberg, Germany
[3] Laboratoire de Radioastronomie Millimétrique (UMR 8112 CNRS), École Normale Supérieure et Observatoire de Paris, 24 rue Lhomond, 75231 Paris, France
[4] Department of Physics and Astronomy, McMaster University, Hamilton, ON L8S 4M1, Canada - Source
Monthly notices of the Royal Astronomical Society (Print). 2011, Vol 414, Num 3, pp 2511-2527, 17 p ; ref : 1 p.1/4
- CODEN
- MNRAA4
- ISSN
- 0035-8711
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- Wiley-Blackwell, Malden, MA
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- ISM: clouds magnetic fields stars: formation turbulence
- Keyword (fr)
- Champ magnétique Densité élevée Diffusion ambipolaire Effondrement Flux magnétique Formation stellaire Masse stellaire Matière interstellaire Nuage moléculaire géant Nuage moléculaire Position Taux croissance Taux formation Transfert masse Turbulence
- Keyword (en)
- Magnetic fields High density Ambipolar diffusion Collapse Magnetic flux Star formation Stellar mass Interstellar matter Giant molecular cloud Molecular clouds Positions Growth rate Formation rate Mass transfer Turbulence
- Keyword (es)
- Densidad elevada Desmoronamiento Nube molecular gigante Grado formación
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 24257784
Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS
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DOI
10.1111/j.1365-2966.2011.18569.x 
https://dx.doi.org/10.1111/j.1365-2966.2011.18569.x
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