Probing the evolving massive star population in Orion with kinematic and radioactive tracers

Astronomy and Astrophysics

Volumn 520, Issue 9, 2010, Pages

  Voss, R ^a,b   Diehl, R ^a   Vink, J S ^c   Hartmann, D H ^d  

^a MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^b EXCELLENCE CLUSTER UNIVERSE   (Germany)

^c ARMAGH OBSERVATORY   (United Kingdom)

^d CLEMSON UNIVERSITY   (United States)

Author keywords

gamma rays: ISM; ISM: abundances; stars: abundances; stars: early type; stars: winds, outflows

Indexed keywords

GAMMA-RAY SIGNAL; INTERSTELLAR MEDIUMS; ISM: ABUNDANCE; ISOCHRONES; MASS LOSS; MASSIVE STARS; OB ASSOCIATION; POPULATION SYNTHESIS; STAR-FORMING REGION; STARS: ABUNDANCES; STARS: EARLY-TYPE; STARS: WINDS, OUTFLOWS; STELLAR CONTENT; UV RADIATION;

ALUMINUM; CHEMICAL ELEMENTS; ELECTRON ENERGY LOSS SPECTROSCOPY; GAMMA RAYS; KINEMATICS; KINETIC ENERGY; RADIOACTIVE TRACERS; RADIOACTIVITY; RADIOISOTOPES; ULTRAVIOLET RADIATION;

STARS;

EID: 78349275036     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014408     Document Type: Article

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