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...

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Main Authors: I. L. Andronov, K. D. Andrych
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2014-10-01
Series:Odessa Astronomical Publications
Subjects:
Online Access:http://oap.onu.edu.ua/article/view/80915
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author I. L. Andronov
K. D. Andrych
author_facet I. L. Andronov
K. D. Andrych
author_sort I. L. Andronov
collection DOAJ
description 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 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.
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spelling doaj.art-c5079bc8c57844bf9876d6f81b5823c82022-12-21T18:15:50ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152014-10-01271384010.18524/1810-4215.2014.27.8091580915DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARSI. L. Andronov0K. D. Andrych1Department “High and Applied Mathematics", Odessa National Maritime UniversityDepartment of Astronomy, Odessa National UniversityThe 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 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.http://oap.onu.edu.ua/article/view/80915stars: variable starsbinary starscataclysmic
spellingShingle I. L. Andronov
K. D. Andrych
DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
Odessa Astronomical Publications
stars: variable stars
binary stars
cataclysmic
title DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
title_full DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
title_fullStr DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
title_full_unstemmed DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
title_short DETERMINATION OF SIZE OF THE EMITTING REGION IN ECLIPSING CATACLYSMIC VARIABLE STARS
title_sort determination of size of the emitting region in eclipsing cataclysmic variable stars
topic stars: variable stars
binary stars
cataclysmic
url http://oap.onu.edu.ua/article/view/80915
work_keys_str_mv AT ilandronov determinationofsizeoftheemittingregionineclipsingcataclysmicvariablestars
AT kdandrych determinationofsizeoftheemittingregionineclipsingcataclysmicvariablestars