Predicted gamma-ray line emission from the Cygnus complex

Astronomy and Astrophysics

Volumn 511, Issue 1, 2010, Pages

  Martin, P ^a,b   Knodlseder J ^a,b   Meynet, G ^c   Diehl, R ^d  

^a CNRS   (France)

^b IRAP   (France)

^c UNIVERSITÉ DE GENÈVE   (Switzerland)

^d MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Gamma rays: ISM; Gamma rays: stars; ISM: bubbles; Nuclear reactions, nucleosynthesis, abundances; Open clusters and associations: individual: Cygnus OB; Stars: early type

Indexed keywords

GAMMA RAYS: STARS; ISM: BUBBLES; NUCLEAR REACTIONS , NUCLEOSYNTHESIS , ABUNDANCES; OPEN CLUSTERS AND ASSOCIATIONS: INDIVIDUAL: CYGNUS OB; STARS: EARLY-TYPE;

ALUMINUM; ASSOCIATION REACTIONS; ASTROPHYSICS; CHEMICAL ELEMENTS; DECAY (ORGANIC); FORECASTING; NUCLEAR ENERGY; NUCLEAR PHYSICS; ROTATION; STARS;

GAMMA RAYS;

EID: 77958022904     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912864     Document Type: Article

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