Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Adygezalzade, A."'
Autor:
N. Z. Ismailov, H. N. Adygezalzade
Publikováno v:
Odessa Astronomical Publications, Vol 28, Iss 2, Pp 227-230 (2016)
By using the archive photometric data’s obtained for a long time intervals we have carried out a master light curves of 28 classical T Tauri type stars. For the physical character of variability mainly 5 type light curves can be separated. We have
Externí odkaz:
https://doaj.org/article/24faed8a7a1448f7aeb0dbb6a59762c4
Publikováno v:
Odessa Astronomical Publications, Vol 23, Iss 0, Pp 46-48 (2010)
Results of the ultraviolet IUE archive spectrum researches of classic T Tauri type star BP Tau had been presented. Spectroscopic parameters of mainly strong emission lines were measured. On the more full massive which had been created on the intensit
Externí odkaz:
https://doaj.org/article/5663321f566c428d93c3299a08cb3096
Autor:
Ismailov, N. ismailovn@yahoo.com, Adygezalzade, A.1
Publikováno v:
Astronomy Reports. Feb2012, Vol. 56 Issue 2, p131-137. 7p. 7 Graphs.
Autor:
H. N. Adygezalzade, N. Z. Ismailov
Publikováno v:
Odessa Astronomical Publications; Том 28, № 2 (2015); 227-230
Odessa Astronomical Publications, Vol 28, Iss 2, Pp 227-230 (2016)
Odessa Astronomical Publications, Vol 28, Iss 2, Pp 227-230 (2016)
By using the archive photometric data’s obtained for a long time intervals we have carried out a master light curves of 28 classical T Tauri type stars. For the physical character of variability mainly 5 type light curves can be separated. We have
Autor:
N. Z. Ismailov, A. N. Adygezalzade
Publikováno v:
Astronomy Reports. 56:131-137
We have analyzed a master light curve of the classical T Tauri star RY Tau. The brightness variations observed in 1983–2004 were found to be periodic. A period of 377 ± 10 d is derived using a frequency analysis. A statistical analysis shows that
Publikováno v:
Odessa Astronomical Publications, Vol 23, Iss 0, Pp 46-48 (2010)
Odessa Astronomical Publications; Том 23 (2010); 46-48
Odessa Astronomical Publications; Том 23 (2010): Odessa Astronomical Publications; 46-48
Odessa Astronomical Publications; Том 23 (2010); 46-48
Odessa Astronomical Publications; Том 23 (2010): Odessa Astronomical Publications; 46-48
Results of the ultraviolet IUE archive spectrum researches of classic T Tauri type star BP Tau had been presented. Spectroscopic parameters of mainly strong emission lines were measured. On the more full massive which had been created on the intensit