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GIANT GAMMA-RAY BUBBLES FROM FERMI-LAT: ACTIVE GALACTIC NUCLEUS ACTIVITY OR BIPOLAR GALACTIC WIND?

Author
MENG SU1 ; SLATYER, Tracy R1 2 ; FINKBEINER, Douglas P1 2
[1] Institute for Theory and Computation, Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, MS-51, Cambridge, MA 02138, United States
[2] Physics Department, Harvard University, Cambridge, MA 02138, United States
Source

The Astrophysical journal. 2010, Vol 724, Num 2, pp 1044-1082, 39 p ; 1 ; ref : 1 p.1/4

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
IOP, Bristol
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
ISM: jets and outflows galaxies: active galaxies: starburst gamma rays: diffuse background
Keyword (fr)
Accrétion Brume Centre galactique Cosmologie Disque galactique Désintégration pion Emission gamma Emission électronique Energétique Galaxies actives Galaxies à flambée Intensité Jet Matière interstellaire Matière sombre Noyau galactique actif Noyau galaxies Proton Rayonnement cosmique Rayonnement gamma Spectre gamma Spectre hyperfréquence Trou noir massif Variation spatiale Vent galactique
Keyword (en)
Accretion Haze Galactic centers Cosmology Galactic disks Pion decay Gamma emission Electron emission Energetics Active galaxies Starburst galaxies Intensity Jets Interstellar matter Dark matter Active galaxy nuclei Galaxy nuclei Protons Cosmic radiation Gamma radiation Gamma spectra Microwave spectra Massive black hole Spatial variation Galactic wind
Keyword (es)
Emisión gamma Energética Galaxias llamarada estelar Intensidad Agujero negro masivo Variación espacial Viento galáctico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
23529801

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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