Показати простий запис статті

dc.contributor.author Bykowski, W.
dc.contributor.author Maciejewski, G.
dc.date.accessioned 2017-06-03T20:11:45Z
dc.date.available 2017-06-03T20:11:45Z
dc.date.issued 2011
dc.identifier.citation Transit timing at Torun Center for Astronomy / W. Bykowski, G. Maciejewski // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 89-91. — Бібліогр.: 11 назв. — англ. uk_UA
dc.identifier.isbn 987-966-439-367-3
dc.identifier.uri http://dspace.nbuv.gov.ua/handle/123456789/119089
dc.description.abstract The transit monitoring is one of well-known methods for discovering and observing new extrasolar planets. Among various advantages, this way of searching other worlds does not require complex and expensive equipment - it can be performed with a relatively small telescope and high-quality CCD camera. At the Center for Astronomy of Nicolaus Copernicus University in Toru«, Poland, we collect observational data using the 60-cm Cassegrain telescope hoping that it would be possible to discover new objects in already known planetary systems using the transit timing variation method. Our observations are a part of a biggercooperation between observatories from many countries. uk_UA
dc.language.iso en uk_UA
dc.publisher Advances in astronomy and space physics uk_UA
dc.relation.ispartof Advances in Astronomy and Space Physics
dc.title Transit timing at Torun Center for Astronomy uk_UA
dc.type Article uk_UA
dc.status published earlier uk_UA


Файли у цій статті

Ця стаття з'являється у наступних колекціях

Показати простий запис статті

Пошук


Розширений пошук

Перегляд

Мій обліковий запис