THE INVESTIGATION OF THE CLASSICAL CEPHEID RT Aur PERIOD

Автор(и)

  • A. S. Kosinsky Amateur group of variable stars observers "Betelgeuse", the Republic Center of Technical Creativity of Pupils, Makaionak street, 12, Minsk 220023 Belarus, Білорусь
  • V. G. Tamello Amateur group of variable stars observers "Betelgeuse", the Republic Center of Technical Creativity of Pupils, Makaionak street, 12, Minsk 220023 Belarus, Білорусь
  • I. J. Kushmar Amateur group of variable stars observers "Betelgeuse", the Republic Center of Technical Creativity of Pupils, Makaionak street, 12, Minsk 220023 Belarus, Білорусь
  • I. S. Bryukhanov Amateur group of variable stars observers "Betelgeuse", the Republic Center of Technical Creativity of Pupils, Makaionak street, 12, Minsk 220023 Belarus, Білорусь
  • A. S. Semenyuta Amateur group of variable stars observers "Betelgeuse", the Republic Center of Technical Creativity of Pupils, Makaionak street, 12, Minsk 220023 Belarus, Білорусь
  • I. I. Balyuk Amateur group of variable stars observers "Betelgeuse", the Republic Center of Technical Creativity of Pupils, Makaionak street, 12, Minsk 220023 Belarus, Білорусь

DOI:

https://doi.org/10.18524/1810-4215.2005.18.98253

Анотація

The outcomes of the research into RT Aur period for the last 93 years are given in the article. New elements of changes in RT Aur brightness have been determined by the authors: J.D.max=2447890,265+3.7283116*E.

Посилання

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2017-04-10

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