Precise mass and radius values for the white dwarf and low mass M dwarf in the pre-cataclysmic binary NN Serpentis

Monthly Notices of the Royal Astronomical Society

Volumn 402, Issue 4, 2010, Pages 2591-2608

  Parsons, S G ^a   Marsh, T R ^a   Copperwheat, C M ^a   Dhillon, V S ^b   Littlefair, S P ^b   Gansicke B T ^a   Hickman, R ^a  

^a UNIVERSITY OF WARWICK   (United Kingdom)

^b UNIVERSITY OF SHEFFIELD   (United Kingdom)

Author keywords

Binaries: eclipsing; Stars: fundamental parameters; Stars: individual: NN Ser; Stars: late type; White dwarfs

Indexed keywords

CCD CAMERAS; IRRADIATION; PHOTOMETRY;

BINARIES:ECLIPSING; HIGH RESOLUTION; LOW-MASS; RADIAL VELOCITY; SECONDARY STARS; STAR: INDIVIDUAL: NN SER; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:FUNDAMENTAL PARAMETERS; STARS:LATE TYPE; VELOCITY AMPLITUDES;

WHITE DWARFS;

EID: 77950936172     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.16072.x     Document Type: Article

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