DE Canum Venaticorum: A bright, eclipsing red dwarf-white dwarf binary

Astronomy and Astrophysics

Volumn 466, Issue 3, 2007, Pages 1031-1041

  Van Den Besselaar, E J M ^a   Greimel, R ^b   Morales Rueda, L ^a   Nelemans, G ^a   Thorstensen, J R ^c   Marsh, T R ^d   Dhillon, V S ^e   Robb, R M ^f   Balam, D D ^f   Guenther, E W ^g   Kemp, J ^h   Augusteijn, T ⁱ   Groot, P J ^a  

^a RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^b ISAAC NEWTON GROUP OF TELESCOPES   (Spain)

^c Lamont Doherty Earth Observatory   (United States)

^d UNIVERSITY OF WARWICK   (United Kingdom)

^e UNIVERSITY OF SHEFFIELD   (United Kingdom)

^f UNIVERSITY OF VICTORIA   (Canada)

^g THÜRINGER LANDESSTERNWARTE TAUTENBURG   (Germany)

^h UNIVERSITY OF HAWAII   (United States)

ⁱ NORDIC OPTICAL TELESCOPE   (Spain)

Author keywords

Stars: binaries: close; Stars: binaries: eclipsing; Stars: fundamental parameters; Stars: individual: DE CVn; Stars: late type; Stars: white dwarfs

Indexed keywords

ASTROPHYSICS; LIGHT EMISSION; PHOTOMETRY; SPECTROSCOPIC ANALYSIS; SPECTRUM ANALYSIS; TEMPERATURE MEASUREMENT;

ECLIPSES; LIGHT CURVES; TIME RESOLVED SPECTROSCOPY; VELOCITY CURVES;

STARS;

EID: 34248562990     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066246     Document Type: Article

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