TIME SERIES ANALYSIS OF THE AFOEV OBSERVATIONS OF SYMBIOTIC STARS UV AUR, TX CVN AND V 1329 CYG

Autor:	L. L. Chinarova, I. L. Andronov, E. Schweitzer
Jazyk:	angličtina
Rok vydání:	2017
Předmět:	lcsh:QB1-991 lcsh:Astronomy Stars Binaries Symbiotic UV Aur TX CVn V 1329 Cyg
Zdroj:	Odessa Astronomical Publications; Том 7 (1994); 103-107 Odessa Astronomical Publications, Vol 7, Iss 1, Pp 103-107 (2017)
ISSN:	1810-4215
Popis:	One frequency sine approximations allowed to obtain the following best fit parameters: periods P = 389.23 ± 0.47d, 3779±73d, 958.7±1.2d mean brightness a = 9.23±0.02m, 9.73±0.01m, 13.26 ±0.07m. semi-amplitudes r = 0.92 ± 0.026m, 0.02 ± 0.007m, 0.49±0.10m and epochs for mean maxima Tm = 2446551.4± 1.8, 7014±21, 5345± 3d for UV Aur, TX CVn and V 1329 Cyg, respectively. Extreme values and cycle lengths vary with time, their characteristics are tabulated.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::6d189d026a8a016318f9a25a85b1c1c9 http://oap.onu.edu.ua/article/view/105728 Zobrazit plný text záznamu