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http://www.mso.anu.edu.au/pfrancis/simulations/XRB.py.
http://www.mso.anu.edu.au/pfrancis/simulations/XRB.py.
81. http://astrometric.sai.msu.ru/articles/Shokin.pdf
... catalogues -----------------------------------------------------------------------577 * 5 00 14.355 -68 54 32.23 1 m fs HV12517 OGLE LMC_SC15 35181 619 5 00 46.136 -69 04 54.40 1 m fs HV5534 OGLE LMC_SC15 81394 626 5 00 55.870 -68 26 20.71 DMA HV2260 634 5 01 05.149 -68 27 05.78 DMA HV2263 635 * 5 01 00.386 -69 03 42.97 DMA HV12524 693 * 5 01 54.611 -68 54 14.06 DMA HV885 OGLE LMC_SC15 148920 700 5 02 01.463 -68 35 02.53 ... The star images were measured on two plates of the astrograph...
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Ссылки http://astrometric.sai.msu.ru/articles/Shokin.pdf -- 114.3 Кб -- 21.11.2000
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82. http://www.astro-soc.odessa.ua/Public-2011.pdf
... 4 .D.Dolgov (INFN, Ferrara, Italy) STOCHASTIC BACKGROUND GRAVITATIONAL WAVES FORM PRIMORDIAL BLACK HOLES OF G.Tsarevsky (PRAO ASC LPI) PROJECT "RADIOASTRON" AND THE FUTURE OF SPACE RADIOASTRONOMY V.N.Melnikov (VNIIMS, Moscow) SCALAR FIELDS AND MULTIDIMENSIONAL MODELS IN GRAVITY AND COSMOLOGY Wednesday, 24.08.2011 Cosmology, Gravitation and High Energy Physics Conference hall "Sovinyon" 09.00 ? ... 8 Section 2. Astrophysics University Recreation Centre "Chernomorka" (2 ) Tuesday, 23.08.2011 14.30 ? ...
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Ссылки http://www.astro-soc.odessa.ua/Public-2011.pdf -- 1027.0 Кб -- 23.07.2014
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83. http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf
... 337, 275292 (2002) The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra S. M. Croom,1 K. Rhook,1 E. A. Corbett,1 B. J. Boyle,1 H. Netzer,2 N. S. Loaring,3 L ... We measure highly significant Baldwin effects for most broad emission lines (C IV 1549, C III] 1909, Mg II 2798, H ,H ) and show that they are predominantly caused by correlations with luminosity, not redshift. ... The correlations of log W with log(1 + z ) for each line. ...
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Ссылки http://www.2dfquasar.org/Papers/2002MNRAS.337..275C.pdf -- 831.9 Кб -- 04.03.2004
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84. http://uranus.sai.msu.ru/~seif/ST10_apj_722_586.pdf
... 1, 2010 Table 3 Best-fit Parameters of the Spectral Analysis of PCA and HEXTE Observation of SS 433 in 3150 keV Energy Rangea Observational ID 10127-01-01-00 10127-01-02-00 10127-01-03-00 10127-01-04-00 10127-01-05-00 10127-01-06-00 10127-01 ... 1.39(1) 1.13(1) 0.99(1) 1.07(1) 0.98(4) 1.17(1) 1.15(3) 1.17(1) 1.21(3) 1.25(6) 1.06(2) 1.09(4) 1.23(1) 1.20(5) 1.07(7) log(A)b 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 2.00 ... Softening of X-ray spectra is seen when the Figure 2. ...
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Ссылки http://uranus.sai.msu.ru/~seif/ST10_apj_722_586.pdf -- 1425.7 Кб -- 23.09.2010
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