Spectral and intensity variations of Galactic °26 Al emission

Astronomy and Astrophysics

Volumn 496, Issue 3, 2009, Pages 713-724

  Wang, W ^a,b   Lang, M G ^a   Diehl, R ^a   Halloin, H ^c   Jean, P ^d   Knodlseder J ^d   Kretschmer, K ^a   Martin, P ^d   Roques, J P ^d   Strong, A W ^a   Winkler, C ^e   Zhang, X L ^a  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d IRAP   (France)

^e EUROPEAN SPACE AGENCY   (Netherlands)

Author keywords

Galaxy: abundances; Gamma rays: observations; ISM: abundances; Nuclear reactions, nucleosynthesis, abundances

Indexed keywords

AL SOURCES; BACKGROUND MODEL; GALACTIC EMISSION; GALACTIC PLANE; GALAXY: ABUNDANCES; GAMMA RAYS: OBSERVATIONS; GAMMA-RAY EMISSION; GAMMA-RAY LINE; HIGH RESOLUTION; INTENSITY VARIATIONS; ISM: ABUNDANCES; LATITUDINAL VARIATION; MASSIVE STARS; NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES; RADIOACTIVE DECAY; SKY DISTRIBUTION; SOURCE REGION; SPATIALLY RESOLVED;

CHEMICAL ELEMENTS; ELECTROMAGNETIC WAVES; EMISSION SPECTROSCOPY; GALAXIES; GAMMA RAYS; INTERCHANGES; NUCLEAR ENERGY; NUCLEAR REACTORS; RADIOACTIVITY; STARS; X RAY CAMERAS;

ALUMINUM;

EID: 65949105696     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200811175     Document Type: Article

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