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dc.contributor.author | Shimansky V. | |
dc.contributor.author | Borisov N. | |
dc.contributor.author | Bikmaev I. | |
dc.contributor.author | Shimanskaya N. | |
dc.date.accessioned | 2018-09-18T20:15:25Z | |
dc.date.available | 2018-09-18T20:15:25Z | |
dc.date.issued | 2012 | |
dc.identifier.issn | 1063-7729 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/138029 | |
dc.description.abstract | We have performed spectroscopy and photometry of eclipses of the pre-cataclysmic variable UUSge using the 6-m telescope of the Special AstrophysicalObservatory and the 1. 5-mRussian-Turkish telescope. Our analysis of variations of the B-V and V-R color indices during the eclipses indicates that the temperature of the secondary is T eff,2 = 6000-6300 K. A similar value, T eff,2 = 6200 ± 200 K, follows from our comparison of the observed spectrum of UU Sge at the total eclipse phase and theoretical spectra of late-type stars. We identify 27 absorption lines of 11 chemical elements in the secondary's spectrum. Their abnormal intensities indicate possible high-velocity turbulent motions (up to ξ turb = 10. 0 km/s) in the atmosphere of the star and the presence of hot gas above its surface. © 2012 Pleiades Publishing, Ltd. | |
dc.relation.ispartofseries | Astronomy Reports | |
dc.title | Observations of eclipses of UU Sge | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 6 | |
dc.relation.ispartofseries-volume | 56 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 456 | |
dc.source.id | SCOPUS10637729-2012-56-6-SID84861884828 |