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,...
Збережено в:
| Опубліковано в: : | Advances in Astronomy and Space Physics |
|---|---|
| Дата: | 2013 |
| Автори: | , , , , , , , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2013
|
| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/119417 |
| Теги: |
Додати тег
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|
| 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| id |
nasplib_isofts_kiev_ua-123456789-119417 |
|---|---|
| record_format |
dspace |
| spelling |
Iłkiewicz, K. Wychudzki, P. Gałan, C. Gładkowski, M. Dobierski, P. Karska, A. Więcek, M. Tomov, T. Mikołajewski, M. 2017-06-06T19:03:20Z 2017-06-06T19:03:20Z 2013 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. 2227-1481 https://nasplib.isofts.kiev.ua/handle/123456789/119417 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. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 |
| spellingShingle |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 Iłkiewicz, K. Wychudzki, P. Gałan, C. Gładkowski, M. Dobierski, P. Karska, A. Więcek, M. Tomov, T. Mikołajewski, M. |
| title_short |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 |
| title_full |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 |
| title_fullStr |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 |
| title_full_unstemmed |
Photometric observations of Epsilon Aurigae during the eclipse of 2009-2011 |
| title_sort |
photometric observations of epsilon aurigae during the eclipse of 2009-2011 |
| author |
Iłkiewicz, K. Wychudzki, P. Gałan, C. Gładkowski, M. Dobierski, P. Karska, A. Więcek, M. Tomov, T. Mikołajewski, M. |
| author_facet |
Iłkiewicz, K. Wychudzki, P. Gałan, C. Gładkowski, M. Dobierski, P. Karska, A. Więcek, M. Tomov, T. Mikołajewski, M. |
| publishDate |
2013 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
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.
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/119417 |
| citation_txt |
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. |
| work_keys_str_mv |
AT iłkiewiczk photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT wychudzkip photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT gałanc photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT gładkowskim photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT dobierskip photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT karskaa photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT wiecekm photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT tomovt photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 AT mikołajewskim photometricobservationsofepsilonaurigaeduringtheeclipseof20092011 |
| first_indexed |
2025-12-02T13:41:11Z |
| last_indexed |
2025-12-02T13:41:11Z |
| _version_ |
1850862655521161216 |