26Al in the inner Galaxy Large-scale spectral characteristics derived with SPI/INTEGRAL

Astronomy and Astrophysics

Volumn 449, Issue 3, 2006, Pages 1025-1031

  Diehl, R ^a   Halloin, H ^a   Kretschmer, K ^a   Strong, A W ^a   Wang, W ^a   Jean, P ^b   Lichti, G G ^a   Knodlseder J ^b   Roques, J P ^b   Schanne, S ^c   Schonfelder V ^a   Von Kienlin, A ^a   Weidenspointner, G ^b   Winkler, C ^d   Wunderer, C ^e  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b IRAP   (France)

^c UNIVERSITÉ PARIS DIDEROT   (France)

^d ESA   (Netherlands)

^e UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Galaxy: abundances; Gamma rays: observations; ISM: abundances; Methods: observational nuclear reactions, nucleosynthesis, abundances

Indexed keywords

ALUMINUM; ATMOSPHERIC SPECTRA; GALAXIES; GAMMA RAYS; GERMANIUM; SPECTROSCOPY; TURBULENCE;

DOPPLER VELOCITY; GALAXY: ABUNDANCES; GAMMA RAYS: OBSERVATIONS; ISM: ABUNDANCES; LARGE-SCALE SPECTRAL CHARACTERISTICS; METHODS: OBSERVATIONAL NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES;

ASTROPHYSICS;

EID: 33645723891     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054301     Document Type: Article

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