Detection of negative superhumps in a low-mass X-ray binary -an end to the long debate on the nature of V1405 Aql (X1916-053)

Monthly Notices of the Royal Astronomical Society

Volumn 330, Issue 2, 2002, Pages

  Retter, A ^a   Chou, Y ^b   Bedding, T R ^a   Naylor, T ^a,c  

^a KEELE UNIVERSITY   (United Kingdom)

^b NATIONAL TSING HUA UNIVERSITY   (Taiwan)

^c UNIVERSITY OF EXETER   (United Kingdom)

Author keywords

Accretion, accretion discs; Novae, cataclysmic variables; X rays: binaries; X rays: individual: V1405 Aq1

Indexed keywords

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; COMPETING MODELS; LIGHT CURVES; LOW-MASS X-RAY BINARIES; NOVAE CATACLYSMIC VARIABLES; ORBITAL PERIODS; X-RAY: INDIVIDUAL: V1405 AQ1; X-RAYS: BINARIES; X-RAYS: INDIVIDUAL;

STARS;

EID: 0041347513     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05280.x     Document Type: Article

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