X-Parsed-By: org.apache.tika.parser.DefaultParser
keywords: Blazars, Gamma-ray emission, Stochastic acceleration, Maxwellian distribution
dc.Type: research-article
dc.Title: HARD GAMMA-RAY SOURCE SPECTRA IN TeV BLAZARS
dc.Source: http://dx.doi.org/10.1142/S2010194512004382
title: HARD GAMMA-RAY SOURCE SPECTRA IN TeV BLAZARS : International Journal of Modern Physics: Conference Series: Vol. 08, No. 
        
    (World Scientific)
dc.Identifier: 10.1142/S2010194512004382
dc.Publisher:  World Scientific Publishing Company 
dc.Language: en
dc.Description: The problem of the hard (intrinsic) ?-ray source spectra in TeV blazars is examined. We show that relativistic Maxwell-like particle distributions provide a suitable interpretation for the inferred hard, very high energy (VHE) photon spectra. We discuss the potential of these distributions to produce broader and softer spectra if multiple zones contribute to the observed emission. We show that the dominance of one component could lead to a VHE flaring state with hard spectral features, like the one observed for Mkn 501 in July 2009.
dc.Format: text/HTML
dc:title: HARD GAMMA-RAY SOURCE SPECTRA IN TeV BLAZARS : International Journal of Modern Physics: Conference Series: Vol. 08, No. 
        
    (World Scientific)
Content-Encoding: UTF-8
Content-Type-Hint: text/html; charset=UTF-8
dc.Creator:  EVA  LEFA 
dc.Date: 2012-04-30
robots: noarchive,nofollow
dc.Coverage: world
dc.Subject: Blazars; Gamma-ray emission; Stochastic acceleration; Maxwellian distribution
Content-Language: en-US
Content-Type: application/xhtml+xml; charset=UTF-8
MSSmartTagsPreventParsing: true