LIGHT CURVE VARIATIONS OF THE MAGNETIC CATACLYSMIC BINARY MR SERPENTIS : PHOTOMETRIC PERIOD IS NOT AS SURE AS BELIEVED

Автор(и)

  • E. P. Pavlenko Crimean Astrophysical Observatory, Nauchny, 334413 Ukraine, Україна
  • N. A. Ketsaris Sternberg State Astronomical Institute, Moscow, 119899 Russia, Російська Федерація
  • A. V. Halevin Department of Astronomy, Odessa State University, 270014 Ukraine, Україна
  • I. L. Andronov Department of Astronomy, Odessa State University, 270014 Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.1994.7.105762

Ключові слова:

Stars, Polars, MR Ser.

Анотація

The light curves show very large even for polars night-to-night variability of the amplitudes (from 0.4m to 1.6m) and shapes. The flares may be owed not only to the inhomogeneous accretion, but possibly some to the UV-Cet events. Large scatter of the phases does not allow to fit all observations even with one period, arguing for future monitoring.

Посилання

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2017-07-01

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