Pressure-confined clumps in magnetized molecular clouds
- Author
- BERTOLDI, F1 ; MCKEE, C. F
[1] Princeton univ. obs., Princeton NJ 08544, United States - Source
The Astrophysical journal. 1992, Vol 395, Num 1, pp 140-157 ; p.1 ; ref : 1/2 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Scientific domain
- Astronomy earth cosmic environment
- Publisher
- University of Chicago Press, Chicago, IL
- Publication country
- United States
- Document type
- Article
- Language
- English
- Keyword (fr)
- Carbone monoxyde Champ magnétique interstellaire Coefficient viriel Confinement Energie gravitationnelle Energie magnétique Molécule interstellaire Nuage moléculaire géant Théorème viriel Turbulence Milieu fragmenté
- Keyword (en)
- Carbon monoxide Interstellar magnetic field Virial coefficient Confinement Gravitational energy Magnetic energy Interstellar molecule Giant molecular cloud Virial theorem Turbulence Clumpy medium
- Keyword (es)
- Carbono monóxido Campo magnético interstelar Coeficiente virial Confinamiento Energía gravitacional Energía magnética Molécula interestelar Nube molecular gigante Teorema del virial Turbulencia Medio fragmento
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D38 Interstellar medium (ism) and nebulae in milky way / 001E03D38D Molecular clouds, h2 clouds, dense clouds, and dark clouds
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 5427545
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
10.1086/171638 
https://dx.doi.org/10.1086/171638
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