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Electron acceleration around the supermassive black hole at the Galactic center

Autor
SIMING LIU1 ; PETROSIAN, Vahé2 ; MELIA, Fulvio3
[1] Center for Space Science and Astrophysics, Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, United States
[2] Department of Physics and Applied Physics, Stanford University, 382 Via Pueblo Mall, Stanford, CA 94305, United States
[3] Department of Physics, 1118 East 4th Street, and Steward Observatory, 933 North Cherry Avenue, University of Arizona, Tucson, AZ 85721, United States
Fuente

The Astrophysical journal. 2004, Vol 611, Num 2, pp L101-L104 ; 2 ; ref : 40 ref

CODEN
ASJOAB
ISSN
0004-637X
Campo Científico
Astronomy earth cosmic environment
Editor
University of Chicago Press, Chicago, IL
País de la publicación
United States
Tipo de documento
Article
Idioma
English
Palabra clave (fr)
Accélération particule Centre galactique Cosmologie Electron cosmique Interaction onde particule Onde plasma Radiosource compacte Radiosource galactique Trou noir supermassif Voie lactée
Palabra clave (in)
Particle acceleration Galactic centers Cosmology Cosmic electrons Particle wave interaction Plasma waves Compact radiosource Galactic radiosource Supermassive black hole Milky Way
Palabra clave (es)
Aceleración partícula Interacción onda partícula Fuente radioeléctrica compacta Radiofuente galáctica Agujero negro supermasivo
Clasificación
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D35 Characteristics and properties of the milky way / 001E03D35J Galactic center, bar, circumnuclear matter, and bulge (including black hole and distance measurements)

Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03D Stellar systems. Galactic and extragalactic objects and systems. The universe / 001E03D70 Unidentified sources and radiation outside the solar system / 001E03D70D Radio sources

Disciplina
Astronomy
Procedencia
Inist-CNRS
Base de datos
PASCAL
Identificador INIST
16172343

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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