DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
The dependencies of the phase of eclipse of the white dwarf’s centre and the durations of the ascending and descending branches of the light curve on the binary system’s parameters were computed using the spherically symmetric approximation and the more accurate model of the elliptical projection on...
| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
Odessa I. I. Mechnykov National University
2014-10-01
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| Series: | Odessa Astronomical Publications |
| Subjects: | |
| Online Access: | http://oap.onu.edu.ua/article/view/80915 |