LIGHT CURVE VARIATIONS OF THE MAGNETIC CATACLYSMIC BINARY MR SERPENTIS : PHOTOMETRIC PERIOD IS NOT AS SURE AS BELIEVED
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 eve...
| Main Authors: | , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Odessa I. I. Mechnykov National University
2017-07-01
|
| Series: | Odessa Astronomical Publications |
| Online Access: | http://oap.onu.edu.ua/article/view/105762 |