Wind accretion in the massive X-ray binary 4U 2206+54: Abnormally slow wind and a moderately eccentric orbit

Astronomy and Astrophysics

Volumn 449, Issue 2, 2006, Pages 687-698

  Ribo M ^a,b   Negueruela, I ^c   Blay, P ^d   Torrejon J M ^c   Reig, P ^e,f  

^a CEA SACLAY   (France)

^b UNIVERSITÉ PARIS DIDEROT   (France)

^c UNIVERSITY OF ALICANTE   (Spain)

^d UNIVERSITY OF VALENCIA   (Spain)

^e INSTITUTE OF ELECTRONIC STRUCTURE AND LASER   (Greece)

^f UNIVERSITY OF CRETE   (Greece)

Author keywords

Stars: emission line, Be; Stars: individual: Bd +53 2790; Stars: variables: general; Stars: winds, outflows; X rays: binaries; X rays: individuals: 4U 2206+54

Indexed keywords

MASS TRANSFER; VELOCITY; WIND EFFECTS; X RAYS;

ECCENTRIC ORBITS; MASS LOSS RATE; STARS EMISSION LINE; STARS VARIABLES GENERAL; STARS WINDS, OUTFLOWS; X-RAY BINARIES; X-RAYS INDIVIDUALS;

ORBITS;

EID: 33645658239     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054206     Document Type: Article

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