Molecular clouds as Cosmic-Ray Barometers

Publications of the Astronomical Society of Japan

Volumn 62, Issue 3, 2010, Pages 769-777

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

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b Astronomy and Astrophysics Section   (Ireland)

^c NAGOYA UNIVERSITY   (Japan)

^d Osaka Prefecture University   (Japan)

^e UNIVERSITY OF ADELAIDE   (Australia)

Author keywords

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

Indexed keywords

CLOUDS; COSMIC RAYS; COSMOLOGY; GERMANIUM COMPOUNDS; HYDROGEN; TELLURIUM COMPOUNDS;

ATOMIC HYDROGEN; COSMIC RAY FLUX; GAMMA-RAYS; HIGH RESOLUTION; HIGH SENSITIVITY; ISM; MOLECULAR CLOUDS; MOLECULAR HYDROGEN; SUPERNOVA REMNANTS; THEORY;

GAMMA RAYS;

EID: 77954793979     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/62.3.769     Document Type: Article

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