Hubble space telescope observations of SV Cam - II. First derivative light-curve modelling using PHOENIX and ATLAS model atmospheres

Monthly Notices of the Royal Astronomical Society

Volumn 367, Issue 3, 2006, Pages 1308-1316

  Jeffers, S V ^a,b   Aufdenberg, J P ^c   Hussain, G A J ^d   Cameron, A Collier ^b   Holzwarth, V R ^b  

^a OBSERVATOIRE MIDI PYRÉNÉES   (France)

^b UNIVERSITY OF ST ANDREWS   (United Kingdom)

^c NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^d EUROPEAN SPACE AGENCY   (Netherlands)

Author keywords

Binaries: eclipsing; Methods: numerical; Stars: activity; Stars: atmospheres; Stars: spots

Indexed keywords

CURVE FITTING; NUMERICAL METHODS; SIGNAL TO NOISE RATIO; SPACE TELESCOPES; STARS;

BINARIES:ECLIPSING; FIRST DERIVATIVE; HUBBLE SPACE TELESCOPES; LIGHT CURVES; METHOD: NUMERICAL; MODEL ATMOSPHERE; SPECIFIC INTENSITY; STAR SPOTS; STAR: ACTIVITY; STARS: ATMOSPHERE;

CAMS;

EID: 33645379450     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10052.x     Document Type: Article

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