Hubble Space Telescope observations of SV Cam - I. The importance of unresolved star-spot distributions in light-curve fitting

Monthly Notices of the Royal Astronomical Society

Volumn 366, Issue 2, 2006, Pages 667-674

  Jeffers, S V ^a,b   Barnes, J R ^b   Cameron, A Collier ^b   Donati, J F ^a  

^a OBSERVATOIRE MIDI PYRÉNÉES   (France)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

Author keywords

Binaries: eclipsing; Stars: activity; Stars: individual: SV Cam; Stars: spots

Indexed keywords

CAMS; CURVE FITTING; SPACE TELESCOPES; STARS;

BINARIES:ECLIPSING; CURVES FITTINGS; HIGH-PRECISION; HUBBLE SPACE TELESCOPES; LIGHT CURVES; SPOT DISTRIBUTION; STAR SPOTS; STAR: ACTIVITY; STAR: INDIVIDUAL: SV CAM; STARS: INDIVIDUAL: PROXIMA CENTAURI;

PHOTOMETRY;

EID: 33645089190     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09905.x     Document Type: Article

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