The VLT-FLAMES tarantula survey: VIII. Multiplicity properties of the O-type star population

Astronomy and Astrophysics

Volumn 550, Issue , 2013, Pages

  Sana, H ^a   De Koter, A ^a,b   De Mink, S E ^c,d   Dunstall, P R ^e   Evans, C J ^f   Henault Brunet V ^g   Maiz Apellaniz J ^h   Ramirez Agudelo O H ^a   Taylor, W D ^g   Walborn, N R ^c   Clark, J S ⁱ   Crowther, P A ^j   Herrero, A ^k,l   Gieles, M ^m   Langer, N ⁿ   Lennon, D J ^c   Vink, J S ^o  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UTRECHT UNIVERSITY   (Netherlands)

^c STScI   (United States)

^d JOHNS HOPKINS UNIVERSITY   (United States)

^e QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^f UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^g UNIVERSITY OF EDINBURGH   (United Kingdom)

^h INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

ⁱ OPEN UNIVERSITY   (United Kingdom)

^j UNIVERSITY OF SHEFFIELD   (United Kingdom)

^k INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^l UNIVERSIDAD DE LA LAGUNA   (Spain)

^m UNIVERSITY OF CAMBRIDGE   (United Kingdom)

ⁿ UNIVERSITY OF BONN   (Germany)

^o ARMAGH OBSERVATORY   (United Kingdom)

more..

Author keywords

Binaries: close; Binaries: spectroscopic; Magellanic Clouds; Open clusters and associations: individual: 30 Dor; Stars: early type; Stars: massive

Indexed keywords

BINARIES: CLOSE; BINARIES: SPECTROSCOPIC; MAGELLANIC CLOUDS; OPEN CLUSTERS AND ASSOCIATIONS; STARS: EARLY-TYPE; STARS: MASSIVE;

GALAXIES; SPECTROSCOPIC ANALYSIS; STATISTICAL MECHANICS; SURVEYS;

STARS;

EID: 84867255900     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201219621     Document Type: Article

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