OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO

We present the review of different properties of several close binary systems, based on our observations. These binaries are as follow: SU UMa type stars V503 Cyg and V1504 Cyg, X-Ray novae V518 Per and V404 Cyg. They have the extremal mass ratio of the primary component to the secondary M1/M2 >...

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Main Authors: Yu. G. Kuznetsova, E. P. Pavlenko, L. M. Sharipova, S. Yu. Shugarov
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2017-02-01
Series:Odessa Astronomical Publications
Online Access:http://oap.onu.edu.ua/article/view/93084
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author Yu. G. Kuznetsova
E. P. Pavlenko
L. M. Sharipova
S. Yu. Shugarov
author_facet Yu. G. Kuznetsova
E. P. Pavlenko
L. M. Sharipova
S. Yu. Shugarov
author_sort Yu. G. Kuznetsova
collection DOAJ
description We present the review of different properties of several close binary systems, based on our observations. These binaries are as follow: SU UMa type stars V503 Cyg and V1504 Cyg, X-Ray novae V518 Per and V404 Cyg. They have the extremal mass ratio of the primary component to the secondary M1/M2 > 3. Some of them show the typical for the SU UMa type stars behaviour, so-called the "positive superhumps" or more rare "negative superhumps". Another display the "forbidden" variability in the ordinary outbursts or the light variation of unknown yet nature.
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spelling doaj.art-4c1575d20f9c4075be8cc20233b51d0c2022-12-22T03:45:38ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-02-0112019720010.18524/1810-4215.1999.12.9308493084OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIOYu. G. Kuznetsova0E. P. PavlenkoL. M. SharipovaS. Yu. ShugarovKiev National University, UkraineWe present the review of different properties of several close binary systems, based on our observations. These binaries are as follow: SU UMa type stars V503 Cyg and V1504 Cyg, X-Ray novae V518 Per and V404 Cyg. They have the extremal mass ratio of the primary component to the secondary M1/M2 > 3. Some of them show the typical for the SU UMa type stars behaviour, so-called the "positive superhumps" or more rare "negative superhumps". Another display the "forbidden" variability in the ordinary outbursts or the light variation of unknown yet nature.http://oap.onu.edu.ua/article/view/93084
spellingShingle Yu. G. Kuznetsova
E. P. Pavlenko
L. M. Sharipova
S. Yu. Shugarov
OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO
Odessa Astronomical Publications
title OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO
title_full OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO
title_fullStr OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO
title_full_unstemmed OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO
title_short OBSERVATIONS OF TYPICAL, RARE AND UNIQUE PHENOMENA IN CLOSE BINARIES WITH EXTREMAL MASS RATIO
title_sort observations of typical rare and unique phenomena in close binaries with extremal mass ratio
url http://oap.onu.edu.ua/article/view/93084
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