Photometric variability of the 1H1936+541 star in 2008-2014

We report the results of observations of the Be/X-ray binary system 1H1936+541. All of the data were obtained on the base of Lisnyky observational station (Astronomical Observatory of the Taras Shevchenko National University of Kyiv) and Southern Station of the Sternberg Astronomical Institute (Lomo...

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Published in:Advances in Astronomy and Space Physics
Date:2014
Main Authors: Simon, A.O., Vasylenko, V.V., Metlova, N.V.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2014
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119807
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Photometric variability of the 1H1936+541 star in 2008-2014 / A.O. Simon, V.V. Vasylenko, N.V. Metlova // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 28-31. — Бібліогр.: 8 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119807
record_format dspace
spelling Simon, A.O.
Vasylenko, V.V.
Metlova, N.V.
2017-06-09T19:45:42Z
2017-06-09T19:45:42Z
2014
Photometric variability of the 1H1936+541 star in 2008-2014 / A.O. Simon, V.V. Vasylenko, N.V. Metlova // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 28-31. — Бібліогр.: 8 назв. — англ.
2227-1481
DOI: 10.17721/2227-1481.4.28-31
https://nasplib.isofts.kiev.ua/handle/123456789/119807
We report the results of observations of the Be/X-ray binary system 1H1936+541. All of the data were obtained on the base of Lisnyky observational station (Astronomical Observatory of the Taras Shevchenko National University of Kyiv) and Southern Station of the Sternberg Astronomical Institute (Lomonosov Moscow State University), giving us three different CCDs in U, B, V, R, and I filters, from 2008 till 2014. During this time, photometrical variability occurred in all bands, however the most significant changes were present in U and I bands. Variabilities in these bands anti-correlate with each other and are in a good agreement with the model of decretion disks around Be stars. Thus, photometric variability claims for changes in the decretion disc structure. Further photometric and spectral observations can help us develop a physical model of this system.
We would like to thank the staff of the Astronomical Observatory of the Taras Shevchenko National University of Kyiv, and that of the Southern Station of the Sternberg Astronomical Institute, for the possibility of the photometric studies with the help of their telescopes and equipment. Special thanks to Ganna Ivashchenko and Oleksiy Agapitov for useful discussions.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Photometric variability of the 1H1936+541 star in 2008-2014
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Photometric variability of the 1H1936+541 star in 2008-2014
spellingShingle Photometric variability of the 1H1936+541 star in 2008-2014
Simon, A.O.
Vasylenko, V.V.
Metlova, N.V.
title_short Photometric variability of the 1H1936+541 star in 2008-2014
title_full Photometric variability of the 1H1936+541 star in 2008-2014
title_fullStr Photometric variability of the 1H1936+541 star in 2008-2014
title_full_unstemmed Photometric variability of the 1H1936+541 star in 2008-2014
title_sort photometric variability of the 1h1936+541 star in 2008-2014
author Simon, A.O.
Vasylenko, V.V.
Metlova, N.V.
author_facet Simon, A.O.
Vasylenko, V.V.
Metlova, N.V.
publishDate 2014
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description We report the results of observations of the Be/X-ray binary system 1H1936+541. All of the data were obtained on the base of Lisnyky observational station (Astronomical Observatory of the Taras Shevchenko National University of Kyiv) and Southern Station of the Sternberg Astronomical Institute (Lomonosov Moscow State University), giving us three different CCDs in U, B, V, R, and I filters, from 2008 till 2014. During this time, photometrical variability occurred in all bands, however the most significant changes were present in U and I bands. Variabilities in these bands anti-correlate with each other and are in a good agreement with the model of decretion disks around Be stars. Thus, photometric variability claims for changes in the decretion disc structure. Further photometric and spectral observations can help us develop a physical model of this system.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119807
citation_txt Photometric variability of the 1H1936+541 star in 2008-2014 / A.O. Simon, V.V. Vasylenko, N.V. Metlova // Advances in Astronomy and Space Physics. — 2014. — Т. 4., вип. 1-2. — С. 28-31. — Бібліогр.: 8 назв. — англ.
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first_indexed 2025-11-29T11:57:39Z
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