The VLT-flames tarantula survey: The fastest rotating O-type star and shortest period LMC pulsar - Remnants of a supernova disrupted binary?

Astrophysical Journal Letters

Volumn 743, Issue 1, 2011, Pages

  Dufton, P L ^a   Dunstall, P R ^a   Evans, C J ^b   Brott, I ^c   Cantiello, M ^d,e   De Koter, A ^f,g   De Mink, S E ^h   Fraser, M ^a   Henault Brunet V ⁱ   Howarth, I D ^j   Langer, N ^d   Lennon, D J ^h   Markova, N ^k   Sana, H ^f   Taylor, W D ⁱ  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^c UNIVERSITY OF VIENNA   (Austria)

^d UNIVERSITY OF BONN   (Germany)

^e UNIVERSITY OF CALIFORNIA   (United States)

^f UNIVERSITY OF AMSTERDAM   (Netherlands)

^g UTRECHT UNIVERSITY   (Netherlands)

^h STScI   (United States)

ⁱ UNIVERSITY OF EDINBURGH   (United Kingdom)

^j UNIVERSITY COLLEGE LONDON   (United Kingdom)

^k BULGARIAN ACADEMY OF SCIENCES   (Bulgaria)

more..

Author keywords

Magellanic Clouds; pulsars: individual (PSR J0537 6910); stars: early type; stars: evolution; stars: rotation

Indexed keywords

EID: 82355163504     PISSN: 20418205     EISSN: 20418213     Source Type: Journal    
DOI: 10.1088/2041-8205/743/1/L22     Document Type: Article

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