Determination of size of the emitting region in eclipsing cataclysmic variable stars
Файли
Дата
2014
Автори
Науковий керівник
Укладач
Редактор
Назва журналу
Номер ISSN
Номер E-ISSN
Назва тому
Видавець
Astroprint
Анотація
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 sphericallysymmetric approximation and the more accurate model of the elliptical projection onto the celestial sphere of the companion (red dwarf) that fills its Roche lobe. The parameters of eclipses in the classical eclipsing polar OTJ
071126+440405 = CSS 081231:071126+440405 were estimated.
Опис
Odessa Astronomical publications / Одесская астроном. обсерватория . – Одесса : Астропринт, 2014 . – Vol.27, I. 1.
Ключові слова
Stars, variable – stars, binary – stars, cataclysmic
Бібліографічний опис
Odessa Astronomical Publications