A long-term optical-X-ray correlation in 4U 1957+11

Monthly Notices of the Royal Astronomical Society

Volumn 402, Issue 4, 2010, Pages 2671-2681

  Russell, D M ^a   Lewis, F ^b,c,d   Roche, P ^b,c,d   Clark, J S ^c   Breedt, E ^e   Fender, R P ^e  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b CARDIFF UNIVERSITY   (United Kingdom)

^c OPEN UNIVERSITY   (United Kingdom)

^d UNIVERSITY OF GLAMORGAN   (United Kingdom)

^e UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

Author keywords

Accretion, accretion discs; Black hole physics; Stars: individual: 4U 1957+11; X rays: binaries

Indexed keywords

BLACK HOLES; GRAVITATION; LEAST SQUARES APPROXIMATIONS; LUMINANCE; NEUTRONS; OPTICAL CORRELATION;

ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; BLACK HOLES; LOW-MASS X-RAY BINARIES; NEUTRON STARS; OPTICAL-; STAR: INDIVIDUAL: 4U 1957+11; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY LUMINOSITY; X-RAYS: BINARIES;

STARS;

EID: 77950957115     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.16098.x     Document Type: Article

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