Modeling the Extragalactic Background Light from Stars and Dust

The extragalactic background light (EBL) from the far-infrared through the visible and extending into the ultraviolet is thought to be dominated by starlight, either through direct emission or through absorption and reradiation by dust. This is the most important energy range for absorbing gamma-ray...

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Veröffentlicht in:	The Astrophysical journal 2010-03, Vol.712 (1), p.238-249
Hauptverfasser:	Finke, Justin D, Razzaque, Soebur, Dermer, Charles D
Format:	Artikel
Sprache:	eng
Schlagworte:	ABSORPTION ANTILEPTONS ANTIMATTER ANTIPARTICLES AROMATICS Astronomy ASTROPHYSICS, COSMOLOGY AND ASTRONOMY COSMIC GAMMA BURSTS COSMIC RADIATION DENSITY DUSTS Earth, ocean, space ELECTROMAGNETIC RADIATION ELECTRONS ELEMENTARY PARTICLES ENERGY DENSITY ENERGY RANGE Exact sciences and technology FERMIONS GALAXIES GAMMA RADIATION GAMMA SPECTRA GEV RANGE GEV RANGE 10-100 HYDROCARBONS IONIZING RADIATIONS LEPTONS LUMINOSITY MAIN SEQUENCE STARS MASS MATTER OPTICAL PROPERTIES ORGANIC COMPOUNDS PHYSICAL PROPERTIES POLYCYCLIC AROMATIC HYDROCARBONS POSITRONS PRIMARY COSMIC RADIATION RADIATIONS RED SHIFT SIMULATION SORPTION SPECTRA STARS TEV RANGE ULTRAVIOLET RADIATION UNIVERSE
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