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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Format: | Article |
Language: | English |
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Odessa I. I. Mechnykov National University
2014-10-01
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Series: | Odessa Astronomical Publications |
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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. |
first_indexed | 2024-12-22T19:05:50Z |
format | Article |
id | doaj.art-c5079bc8c57844bf9876d6f81b5823c8 |
institution | Directory Open Access Journal |
issn | 1810-4215 |
language | English |
last_indexed | 2024-12-22T19:05:50Z |
publishDate | 2014-10-01 |
publisher | Odessa I. I. Mechnykov National University |
record_format | Article |
series | Odessa Astronomical Publications |
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 |