Zobrazeno 1 - 5
of 5
pro vyhledávání: '"D. S. Senio"'
Autor:
I. L Andronov, K. Arai, L. L. Chinarova, N. I. Dorokhov, T. N. Dorokhova, A. Dumitrescu, D. Nogami, S. V. Kolesnikov, A. Lepardo, P. A. Mason, K. Matsumoto, G. Oprescu, G. Pajdosz, R. Passuelo, L. Patkos, D. S. Senio, G. Sostero, V. F. Suleimanov, J. Tremko, G. V. Zhukov, S. Zola
Publikováno v:
Odessa Astronomical Publications, Vol 10, Iss 0, Pp 10-14 (2017)
Results obtained during the international observational campaign ” Т Т Ari-94” are briefly discussed. During 258 hours, totally 51299 observations were obtained in 12 observatories. The moments of 68 individual maxima and 74 minima are tabulate
Externí odkaz:
https://doaj.org/article/823ef66593684429847a6acbe9b3fd73
Publikováno v:
Odessa Astronomical Publications, Vol 9, Iss 0, Pp 57-58 (2017)
Simultaneous WBVR photometric observations of TT Ari during 94 / 95 years are presented. The periodogram analysis of the obtained light curves and colours are curried out. The photometric period equal 3.2 h and its one day aliases are found from ligh
Externí odkaz:
https://doaj.org/article/b3aeafd6920d41ec80a666e8da9e28ab
Autor:
G. V. Zhukov, I. F. Bikmaev, N. A. Sakhibullin, D. S. Senio, I. M. Khamitov, A. I. Belova, I. Yu. Belov, Valery F. Suleimanov
Publikováno v:
Astronomy Letters. 39:111-125
We present the results of photometric observations of a bright cataclysmic variable TT Ari with an orbital period of 0.13755 days. CCD observations were carried out with the Russian-Turkish RTT 150 telescope in 2001 and 2004 (13 nights). Multi-color
A Search for Periodic and Quasi-periodic Photometric Behavior in the Cataclysmic Variable TT Arietis
Autor:
Paul A. Mason, T. N. Dorokhova, Daisaku Nogami, Valery F. Suleimanov, G. Oprescu, A. Lepardo, D. S. Senio, J. Tremko, N. I. Dorokhov, G. V. Zhukov, L. Patkos, Katsura Matsumoto, Alexandru Dumitrescu, Ivan L. Andronov, Sergey Kolesnikov, K. Arai, Lidia L. Chinarova, G. Pajdosz, Staszek Zola, G. Sostero, R. Passuelo
Publikováno v:
The Astronomical Journal. 117:574-586
Observations of TT Ari obtained at 11 observatories (campaign TT Ari–94) during 258 hr were carried out to study optical variability on timescales from minutes to weeks. The best-fit primary photometric period determined from 16 nights of data obta
Publikováno v:
Astronomical & Astrophysical Transactions. 15:117-130
Four-colour photometric observations of TT Ari and V603 Aql in 1994–1995 are presented. Both stars show photometric periodicities in their light curves, 3.2 h and 3.5 h respectively. But their colours sometimes also vary with spectroscopic periods