Does the blazar gamma-ray spectrum harden with increasing flux? Analysts of 9 years of egret data
- Auteur
- NANDIKOTKUR, Giridhar1 2 ; JAHODA, Keith M2 ; HARTMAN, R. C2 ; MURHERJEE, R3 ; SREEKUMAR, P4 ; BOTTCHER, M5 ; SAMBRUNA, R. M2 ; SWANK, Jean H2
[1] Department of Physics, University of Maryland at College Park, College Park, MD, United States
[2] Exploration of the Universe Division, NASA Goddard Space Flight Center, Greenbelt, MD, United States
[3] Department of Physics and Astronomy, Barnard College and Columbia University, New York, NY, United States
[4] Space Astronomy and Instrumentation Division, ISRO Satellite Centre, Bangalore, Kamataka, India
[5] Astrophysical Institute, Department of Physics and Astronomy, Ohio University, Athens, OH, United States - Source
The Astrophysical journal. 2007, Vol 657, Num 2, pp 706-724, 19 p ; 1 ; ref : 1/2 p
- CODEN
- ASJOAB
- ISSN
- 0004-637X
- Domaine scientifique
- Astronomy earth cosmic environment
- Editeur
- University of Chicago Press, Chicago, IL
- Pays de publication
- United States
- Type de document
- Article
- Langue
- English
- Mot clé auteur
- galaxies: active methods: data analysis methods: statistical radiation mechanisms: nonthermal
- Mot clé (fr)
- Analyse donnée Blazar Galaxies actives Mécanisme rayonnement Méthode statistique Rayonnement gamma Rayonnement non thermique Spectre gamma
- Mot clé (en)
- Data analysis Blazar Active galaxies Radiation mechanism Statistical method Gamma radiation Nonthermal radiation Gamma spectra
- Mot clé (es)
- Mecanismo radiación Método estadístico
- Classification
- Discipline
- Astronomy
- Provenance
- Inist-CNRS
- Base de données
- PASCAL
- Identifiant INIST
- 18626490
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
10.1086/510795 
https://dx.doi.org/10.1086/510795
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