... 1987. .3, , 5. . ... 90 Vd lgE N: 1 ­ N=1010, 2 ­ N=1011, 3 ­ N=1012 , 4 ­ N=1013 -3. ... L1 , , , V, / , V0, / , N 1010, -3 4 000 L2 13 000 L3 25 000 L5 45 000 L6 43 000 L7 37 000 L8 10 000 37 000 29 000 20 000 2 000 -13 000 -20 000 -41 000 7,3 14,6 25,1 -8,5 -29,7 -35,7 -77,7 36,5 67,3 124,8 76,4 33,8 39,2 93,9 7,41 6,92 4,79 7,59 3,31 3,02 6,31 Vd lgE : 1 ­ N=1010; 2 ­ N=1011; 3 ­ N=1012; 4 ­ N=1013 -3 "" . ... 7,6], , 7000 ­ 20 000 1 в 1011 ­ 6 в 1012 -3. 10-5 ­ 10-3 /, 20 170 /. 5 в 1012 -3 . ...

... Salyut-7 . ... Salyut-3/5 (Almaz) . ... Salyut-6/7 with . ... Proton with Salyut-2 . Inside Salyut-6 . Salyut-6 trainer . Central control post. Hatch to the transfer compartment is also visible. Note: left part of the control panel is an exact copy of Soyuz panel. ... Backward view from the very front of working compartment. Extendable shower (see below) is seen in upper left corner. ... Extendable shower . ...

The Second U.S. Naval Observatory CCD Astrograph Catalog ( UCAC2 ) Table of Contents 1) Introduction 2) Summary of the Project a) Observations and Instrumentation b) Reductions of UCAC Observations c) Computation of Proper Motions 3) Properties of the Catalog and Important Notes For the User a) Sky Coverage b) Completeness c) Positions, Proper Motions and Error Calculations d) UCAC2 Magnitudes e) 2MASS Photometry f) Non-stellar ... All stars in the UCAC2 have proper motions. ...

... Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (1­22 GHz) spectra obtained on the RATAN­600 radio telescope at epochs close to those of the VLBI observations. ... The image (Fig. 5) shows that the source structure at 18 cm is compact, consisting of a VLBI core and two jet components, with the outer component lying 5 mas (30 pc) to the northwest of the core ( = 54 ). ...

... Under certain conditions, like those in the nucleus of a QSO, all atoms can be made to emit light at particular wavelengths. ... If that source is approaching the observer, the wave is squashed up onto itself making the wavelength shorter. ... This is redshift. ... You can see how the section of the QSO spectrum which we observe changes with redshift. ... We then see how far we had to slide the observed spectrum along the scale to make it match and that is the objects redshift. ... The 2QZ team . ...

... 16-mm/2.8 Fish-eye . ... I set up my Edixa Prismaflex TTL on a tripod outside the dome at Zeiss 50" and opened the camera for several hours. The 2.6 m Shain reflector is visible at center. The time exposure of about 5 hours duration showing circumpolar stars. The dome can be seen to blur slightly due to their motion during the exposure. Back to Astronomical Images Home Page . ...