Correlated X-ray and optical variability in V404 Cygni in quiescence

Astrophysical Journal

Volumn 611, Issue 2 II, 2004, Pages

  Hynes, R I ^a   Charles, P A ^b   Garcia, M R ^c   Robinson, E L ^a   Casares, J ^d   Haswell, C A ^e   Kong, A K H ^c   Rupen, M ^f   Fender, R P ^g   Wagner, R M ^h   Gallo, E ^g   Eves, B A C ^e   Shahbaz, T ^d   Zurita, C ⁱ  

^a The University of Texas at Austin   (United States)

^b UNIVERSITY OF SOUTHAMPTON   (United Kingdom)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^e OPEN UNIVERSITY   (United Kingdom)

^f NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^g UNIVERSITY OF AMSTERDAM   (Netherlands)

^h UNIVERSITY OF ARIZONA   (United States)

ⁱ UNIVERSITY OF LISBON   (Portugal)

Author keywords

Accretion, accretion disks; Binaries: close; Stars: individual (V404 Cygni); X rays: binaries

Indexed keywords

EID: 5644234202     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/424005     Document Type: Article

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