Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011

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,...

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Published in:Advances in Astronomy and Space Physics
Date:2013
Main Authors: Iłkiewicz, K., Wychudzki, P., Gałan, C., Gładkowski, M., Dobierski, P., Karska, A., Więcek, M., Tomov, T., Mikołajewski, M.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2013
Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/119417
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this: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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine