Using population synthesis of massive stars to study the interstellar medium near OB associations

Astronomy and Astrophysics

Volumn 504, Issue 2, 2009, Pages 531-542

  Voss, R ^a,b   Diehl, R ^a   Hartmann, D H ^c   Cervino M ^d   Vink, J S ^e   Meynet, G ^f   Limongi, M ^g   Chieffi, A ^g  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b EXCELLENCE CLUSTER UNIVERSE   (Germany)

^c CLEMSON UNIVERSITY   (United States)

^d INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

^e ARMAGH OBSERVATORY   (United Kingdom)

^f UNIVERSITÉ DE GENÈVE   (Switzerland)

^g INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

Author keywords

Gamma rays: observations; ISM: abundances; Stars: abundances; Stars: early type; Stars: winds, outflows

Indexed keywords

GAMMA RAYS: OBSERVATIONS; ISM: ABUNDANCES; STARS: ABUNDANCES; STARS: EARLY-TYPE; STARS: WINDS, OUTFLOWS;

ASSOCIATION REACTIONS; COMPUTER SIMULATION; ELECTROMAGNETIC WAVES; ELECTRON ENERGY LOSS SPECTROSCOPY; GAMMA RAYS; HYDROGEN; ISOTOPES; KINETIC ENERGY; MONTE CARLO METHODS; POPULATION STATISTICS; RADIOISOTOPES; ROTATION; WIND; WIND POWER; X RAY CAMERAS;

STARS;

EID: 70349315252     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200912260     Document Type: Article

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