HOT SELF-SIMILAR RELATIVISTIC MAGNETOHYDRODYNAMIC FLOWS
- Author
- ZAKAMSKA, Nadia L1 ; BEGELMAN, Mitchell C2 3 ; BLANDFORD, Roger D4
[1] Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, United States
[2] JILA, 440 UCB, University of Colorado at Boulder, Boulder, CO 80309-0440, United States
[3] Department of Astrophysical and Planetary Sciences, University of Colorado at Boulder, Boulder, CO 80309-0440, United States
[4] KIPAC, Stanford University, 2575 Sand Hill Road, Menlo Park, CA 94025, United States - Source
The Astrophysical journal. 2008, Vol 679, Num 2, pp 990-999, 10 p ; 1 ; ref : 1/4 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
- Author keyword
- MHD galaxies: jets radio continuum: galaxies
- Keyword (fr)
- Continuum Ecoulement relativiste Galaxies Jet Magnétohydrodynamique relativiste Radiogalaxies Radiosource cosmique
- Keyword (en)
- Continuum Relativistic flow Galaxies Jets Relativistic magnetohydrodynamics Radio galaxies Cosmic radio sources
- Keyword (es)
- Continuo Flujo relativista Magnetohidrodinámica relativista
- Classification
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20390070
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
10.1086/587870 
https://dx.doi.org/10.1086/587870
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