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

• Veröffentlicht in: Advances in Astronomy and Space Physics
• Datum: 2013
• Hauptverfasser: Iłkiewicz, K., Wychudzki, P., Gałan, C., Gładkowski, M., Dobierski, P., Karska, A., Więcek, M., Tomov, T., Mikołajewski, M.
• Format: Artikel
• Sprache: Englisch
• Veröffentlicht: Головна астрономічна обсерваторія НАН України 2013
• Online Zugang: https://nasplib.isofts.kiev.ua/handle/123456789/119417
• Назва журналу: Digital Library of Periodicals of National Academy of Sciences of Ukraine
• Zitieren: 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.

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,...