Zobrazeno 1 - 8
of 8
pro vyhledávání: '"I. Nikoloff"'
Publikováno v:
Icarus. 35:344-359
Results of UBV photometry and polarimetry of 1580 Betulia during its 1976 apparition are presented. The synodic period of rotation is found to be 6.130 hr. The linear phase coefficient and absolute magnitude of the primary maximum in V are 0.032 mag/
Autor:
A. E. Vaughan, O. B. Slee, I. Nikoloff, G. J. Nelson, Michael C. B. Ashley, A. R. Hyland, R. D. Robinson, Ian R. Tuohy
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 220:91-106
Autor:
E. Marcus, W. Gliese, I. Nikoloff, B. L. Klock, H. I. Potter, K. N. Tavastsherna, R. H. Tucker, G. Teleki, S. Débarbat, H. J. Fogh Olsen, C. C. Counselman, C. A. Murray, H. Wood, Erik Høg
Publikováno v:
International Astronomical Union Colloquium. 48:545-556
SummaryThe paper presents various views of the future of fundamental astrometry, arranged under the following headings:1 General and Introductory Remarks2 The New Techniques2.1 Modernised Classical Astrometry2.2 Laser Ranging2.3 Radio Astrometry2.4 S
Autor:
Erik Høg, Luo Ding-jiang, J A Opez, H Yasuda, J A Hughes, K. N. Tavastsherna, Y S Yatskiv, C A Anguita, G. Teleki, Walter Fricke, I. Nikoloff, G Billaud, B. L. Klock, R. H. Tucker, S. Débarbat
Publikováno v:
Transactions of the International Astronomical Union. 18:33-42
It is with deep regret that we mention the death, on 15 July 1969, of Prof. Dr G. Demetrescu who has done so much for the development of Astronomy in Roumania. This report is based on letters received from members of the Commission, whom I wish to th
Autor:
Erik Høg, I. Nikoloff
Publikováno v:
Symposium - International Astronomical Union. 61:79-84
A total of 110000 observations of 26000 stars was obtained between 1967 and 1972. The internal mean errors are 0″.17 and 0″.27 in Δα cosδ and Δδ, respectively, both multiplied by the factor (cosz)−0.5 at the zenith distance z. The prelimin
Publikováno v:
Publications of the Astronomical Society of Australia. 1:207-208
The naked-eye cluster, Messier 7, is situated in the constellation of Scorpius, south of the great Sagittarius star clouds, and close to the galactic centre.
Autor:
Jeffrey L. Linsky, B. C. Siegman, O. B. Slee, P. J. Quinn, D. Harwood, A. Verveer, M. Candy, B. M. Haisch, I. Nikoloff, I. R. G. Wilson
Publikováno v:
The Astrophysical Journal. 245:1009
We report on a coordinated program involving X-ray, ultraviolet, optical, and radio observations of the dM5e flare star Proxima Centauri. We detected one major X-ray flare event with L/sub x/(0.2--4.0 keV)roughly-equal6.0 x 10/sup 27/ ergs s/sup -1/,
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