Modeling the gamma-ray emission produced by runaway cosmic rays in the environment of RX J1713.7-3946

Publications of the Astronomical Society of Japan

Volumn 62, Issue 5, 2010, Pages 1127-1134

  Casanova, Sabrina ^a   Jones, David I ^a   Aharonian, Felix A ^a,b   Fukui, Yasuo ^c   Gabici, Stefano ^b,d   Kawamura, Akiko ^c   Onishi, Toshikazu ^c   Rowell, Gavin ^e   Sano, Hidetoshi ^c   Torii, Kazufumi ^c   Yamamoto, Hiroaki ^c  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^c NAGOYA UNIVERSITY   (Japan)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e UNIVERSITY OF ADELAIDE   (Australia)

Author keywords

Gamma rays: Theory; ISM: Clouds ISM: Cosmic rays; ISM: Supernova remnants

Indexed keywords

COSMOLOGY; GAMMA RAYS; GERMANIUM COMPOUNDS; SUPERNOVAE; TELLURIUM COMPOUNDS;

CLOUDS-ISM; GAMMA RAYS: THEORY; GAMMA-RAY EMISSION; GAMMA-RAYS; ISM : CLOUDS; ISM: CLOUD-ISM: COSMIC RAY; ISM: COSMIC RAYS; ISM: SUPERNOVA REMNANTS; RX J1713.7-3946; SUPERNOVA REMNANTS;

COSMIC RAYS;

EID: 79251519668     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/62.5.1127     Document Type: Article

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