Early SPI/INTEGRAL constraints on the morphology of the 511 KeV line emission in the 4th galactic quadrant

Astronomy and Astrophysics

Volumn 411, Issue 1, 2003, Pages

  Knodlseder J ^a   Lonjou, V ^a   Jean, P ^a   Allain, M ^a   Mandrou, P ^a   Roques, J P ^a   Skinner, G K ^a   Vedrenne, G ^a   Von Ballmoos, P ^a   Weidenspointner, G ^a,e   Caraveo, P ^d   Cordier, B ^c   Schonfelder V ^b   Teegarden, B J ^e  

^a CNRS   (France)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c CEA SACLAY   (France)

^d INAF IASF MILANO   (Italy)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Gamma rays; Observations

Indexed keywords

COMPUTER SIMULATION; DATA REDUCTION; GAMMA RAYS; IMAGING SYSTEMS; MATHEMATICAL MODELS; MONTE CARLO METHODS; SPACECRAFT OBSERVATORIES; SPECTROSCOPIC ANALYSIS;

GALACTIC DISK COMPONENTS; SPATIAL DISTRIBUTIONS;

ASTROPHYSICS;

EID: 10744221575     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031437     Document Type: Article

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