The 1998 outburst of XTE J1550-564: A model based on multiwavelength observations

Astrophysical Journal

Volumn 565, Issue 2 I, 2002, Pages 1161-1168

  Wu, K ^a,b   Soria, R ^a   Campbell Wilson, D ^b   Hannikainen, D ^c   Harmon, B A ^d   Hunstead, R ^b   Johnston, H ^b   McCollough, M ^d   McIntyre, C ^b,e  

^a UNIVERSITY COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF SYDNEY   (Australia)

^c UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^d NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^e CSIRO   (Australia)

Author keywords

Accretion, accretion disks; Binaries: close; Black hole physics; Stars: individual (XTE J1550 564); Stars: magnetic fields; X rays: stars

Indexed keywords

EID: 0041672506     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324328     Document Type: Article

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