A photometric-spectroscopic analysis and the evolutionary status of the Algol-type binary U Coronae Borealis

Monthly Notices of the Royal Astronomical Society

Volumn 342, Issue 4, 2003, Pages 1349-1360

  Yerli, S K ^a,b   Sarna, M J ^a,b,c   Zola, S ^d,e   Smith, Robert Connon ^a   Tovmassian, G ^f  

^a UNIVERSITY OF SUSSEX   (United Kingdom)

^b MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^c NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^d JAGIELLONIAN UNIVERSITY   (Poland)

^e PEDAGOGICAL UNIVERSITY   (Poland)

^f UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Binaries: eclipsing; Binaries: spectroscopic; Stars: abundances; Stars: evolution; Stars: individual: U Coronae Borealis

Indexed keywords

STARS;

BINARIES: SPECTROSCOPIC; BINARIES:ECLIPSING; BOREALIS; RADIAL VELOCITY; SECONDARY COMPONENTS; STAR: EVOLUTION; STAR: INDIVIDUAL: U CORONA BOREALI; STARS ABUNDANCES; STARS: BE; STARS: INDIVIDUAL: PROXIMA CENTAURI;

SPECTROSCOPIC ANALYSIS;

EID: 0142105404     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06644.x     Document Type: Article

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