Forward modelling of Kepler-band variability due to faculae and spots
نویسندگان
چکیده
منابع مشابه
The activity pattern on MM Herculis: spots and faculae
The RS CVn type eclipsing binary MM Herculis was observed using B, V, and R filters in 1997 and the light and colour curves were obtained. The long-term (1976–1997) variations in the brightness and colour of the system were revealed by examining 12 light and colour curves. The reason for the variations in the B–V colour curves may be the photospheric bright facular structures that surround star...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 2021
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/stab1190