## Abstract We present more than 1000βday long photometry of EY Draconis in __BV__ (__RI__)~C~ passbands. The changes in the light curve are caused by the spottedness of the rotating surface. Modelling of the spotted surface shows that there are two large active regions present on the star on the o
β¦ LIBER β¦
Results of the photometry of the spotted dM1-2e star EY Draconis
β Scribed by K. Vida
- Publisher
- John Wiley and Sons
- Year
- 2007
- Tongue
- English
- Weight
- 636 KB
- Volume
- 328
- Category
- Article
- ISSN
- 0004-6337
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