Field O stars: Formed in situ or as runaways?

Monthly Notices of the Royal Astronomical Society

Volumn 424, Issue 4, 2012, Pages 3037-3049

  Gvaramadze, V V ^a,b   Weidner, C ^c,d   Kroupa, P ^e   Pflamm Altenburg, J ^e  

^a MOSCOW STATE UNIVERSITY   (Russian Federation)

^b Isaac Newton Institute of Chile   (Russian Federation)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d UNIVERSITY OF ST ANDREWS   (United Kingdom)

^e UNIVERSITY OF BONN   (Germany)

Author keywords

Galaxies: star formation; Magellanic Clouds; Stars: early type; Stars: formation; Stars: kinematics and dynamics; Stars: massive

Indexed keywords

SEARCH ENGINES; SUPERNOVAE; VELOCITY;

GALAXIES: STAR FORMATION; MAGELLANIC CLOUDS; MASSIVE STARS; MILKY WAYS; SPACE-VELOCITY; STAR CLUSTERS; STAR KINEMATICS AND DYNAMICS; STARS FORMATION; STARS: MASSIVE; STARS:EARLY TYPE;

GALAXIES;

EID: 84864946179     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2012.21452.x     Document Type: Article

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