| dc.contributor.author | Zejda, Miloslav | |
| dc.contributor.author | Mikulášek, Zdeněk | |
| dc.contributor.author | Zhu, L.-Y. | |
| dc.contributor.author | Qian, Sheng-Bang | |
| dc.contributor.author | Liška, Jiří | |
| dc.contributor.author | Janík, Jan | |
| dc.date.accessioned | 2015-01-19T14:33:41Z | |
| dc.date.available | 2015-01-19T14:33:41Z | |
| dc.date.issued | 2014 | |
| dc.identifier.citation | Contributions of the Astronomical Observatory Skalnaté Pleso. 2014, vol. 43, no. 3, p. 462-464. | cs |
| dc.identifier.issn | 1335-1842 | |
| dc.identifier.issn | 1336-0337 | |
| dc.identifier.uri | http://hdl.handle.net/10084/106319 | |
| dc.description.abstract | V1010 Oph is a relatively bright near contact binary. We present
a new study including four-colour photometry and a model of the system. The
uniqueness of our study is in the using of only a centimetre-class telescope with
a CCD camera. We show that such small, cheap equipment seems to be very
helpful in the investigation of bright variable stars. | cs |
| dc.language.iso | en | cs |
| dc.publisher | Astronomický ústav Slovenskej akadémie vied | cs |
| dc.relation.ispartofseries | Contributions of the Astronomical Observatory Skalnaté Pleso | cs |
| dc.relation.uri | http://www.ta3.sk/caosp/Eedition/FullTexts/vol43no3/pp462-464.pdf | cs |
| dc.title | V1010 Oph investigated by a cm-class telescope | cs |
| dc.type | article | cs |
| dc.type.status | Peer-reviewed | cs |
| dc.description.source | Web of Science | cs |
| dc.description.volume | 43 | cs |
| dc.description.issue | 3 | cs |
| dc.description.lastpage | 464 | cs |
| dc.description.firstpage | 462 | cs |
| dc.identifier.wos | 000338483100066 | |