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dc.contributor.author |
Iłkiewicz, K. |
|
dc.contributor.author |
Wychudzki, P. |
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dc.contributor.author |
Gałan, C. |
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dc.contributor.author |
Gładkowski, M. |
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dc.contributor.author |
Dobierski, P. |
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dc.contributor.author |
Karska, A. |
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dc.contributor.author |
Więcek, M. |
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dc.contributor.author |
Tomov, T. |
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dc.contributor.author |
Mikołajewski, M. |
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dc.date.accessioned |
2017-06-06T19:03:20Z |
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dc.date.available |
2017-06-06T19:03:20Z |
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dc.date.issued |
2013 |
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dc.identifier.citation |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 / K. Iłkiewicz, P. Wychudzki, C. Gałan, M. Gładkowski, P. Dobierski, A. Karska, M. Więcek, T. Tomov, M. Mikołajewski // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 23-28. — Бібліогр.: 5 назв. — англ. |
uk_UA |
dc.identifier.issn |
2227-1481 |
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dc.identifier.uri |
http://dspace.nbuv.gov.ua/handle/123456789/119417 |
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dc.description.abstract |
Epsilon Aurigae is a bright binary system, in which an F0 supergiant is eclipsed by a dark disk around the companion, every 27.1 years. Although the star has been observed and studied for nearly two centuries, it remains an usolved mystery. For the latest ε Aur eclipse, which occurred in 2009-2011, an international observing campaign was organized. In this publication, multicolor BV R photometric observations obtained in the framework of this campaign, are presented. Part of these data have been corrected for atmospheric extinction and transformed to the standard Johnson's photometric system. |
uk_UA |
dc.language.iso |
en |
uk_UA |
dc.publisher |
Головна астрономічна обсерваторія НАН України |
uk_UA |
dc.relation.ispartof |
Advances in Astronomy and Space Physics |
|
dc.title |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 |
uk_UA |
dc.type |
Article |
uk_UA |
dc.status |
published earlier |
uk_UA |
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