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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| Опубліковано в: : | Advances in Astronomy and Space Physics |
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| Дата: | 2013 |
| Автори: | , , , , , , , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2013
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| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/119417 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | 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. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| Резюме: | 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.
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| ISSN: | 2227-1481 |