HST and ground-based eclipse observations of V2051 Ophiuchi: Binary parameters

Monthly Notices of the Royal Astronomical Society

Volumn 300, Issue 1, 1998, Pages 233-243

  Baptista, Raymundo ^a   Catalan M S ^b   Horne, Keith ^c   Zilli, D ^a  

^a FEDERAL UNIVERSITY OF SANTA CATARINA   (Brazil)

^b KEELE UNIVERSITY   (United Kingdom)

^c UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Binaries: close; Eclipses; Novae, cataclysmic variables; Stars: individual: V2051 oph; Ultraviolet: stars

Indexed keywords

ELECTROMAGNETIC WAVE EMISSION; WHITE DWARFS;

BINARIES: CLOSE; DWARF NOVAE; ECLIPSE; EMISSION LINES; GROUND BASED; LIGHT CURVES; NOVAE CATACLYSMIC VARIABLES; STAR: INDIVIDUAL: V2051 OPH; STARS: INDIVIDUAL: PROXIMA CENTAURI; ULTRAVIOLET: STARS;

PHOTOMETRY;

EID: 0000246948     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01887.x     Document Type: Article

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