AY LYRAE SUPERHUMPS PHOTOMETRY

Автор(и)

  • V. P. Smykov Astrophysical Observatory, Moldova State University, str. Mateevich 60, 277014, Kishinev, Moldova, Республіка Молдова

DOI:

https://doi.org/10.18524/1810-4215.1994.7.105788

Ключові слова:

Stars, Dwarf Novae, Binaries

Анотація

During the superoutburst the superhumps with an amplitude of 0.2 mag in BV were observed. The superhumps period changed from 90 min at the maximum of the outbursts (12.8 V) up to 108 min at V = 13.2. These values are less than that obtained by previous authors.

Посилання

Khrusina T.S., Shugarov S.Yu.: 1991, Atlas of cataclysmic variables. U Geminorum stars, Moscow University Press.

Patterson J.: 1979, A J., 84, 804.

Szymanski M., Udalski A.: 1987, I.B.V.S., 3105.

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Опубліковано

2017-07-01

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