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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 |
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dc.date.issued |
2011 |
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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 |
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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 |
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