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We show that by using small telescopes with mirror diameters up to 1.25 m and even 6 cm photo lens, it is possible to carry out qualitative observations and obtain a new information about variable stars. We have studied in detail and now present photometric behavior of a dwarf nova OV Boo, undergoing outburst in the middle of March 2017.
№ | Имя | Описание | Имя файла | Размер | Добавлен |
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1. | Презентация | final.ppt | 613,5 КБ | 15 ноября 2017 [s_shugarov] |