... Field of research: Extragalactic astronomy. ... NASA Astrophysics Data System (ADS) Abstract Service . ... CADC Home Page . ... CCD Images of Galaxies . ... RUSSIAN LINKS . ... UA Astronomy Personal Home Page - Bill Keel . ... The Shape of the Rotation Curves of Edge-on Galaxies, by A.V.Zasov and A.V.Khoperskov, 2003. ... A Thickness of Stellar Discs, by A.V.Zasov, and D.V.Bizyaev, 2003 . Minimum Velocity Dispersion in Stable Stellar Disks, by A.V.Khoperskov, A.V.Zasov, and N.V.Tyurina, 2003 . ...

Comment on J0627-3529 . We have detected the core of an FR-I object and early-type galaxy (Venturi et al. 1995). The core is 0.54 Jy at 2.3 GHz on the Parkes-Tidbinbilla baseline (Morganti et al. 1997) and 0.6 Jy at 5 GHz (VLA data, Ekers et al. (1989) and Morganti, Killeen & Tadhunter (1993)). The VLBA image at 2.3 GHz with the resolution of 15x9 mas shows a "core-jet" structure, with the core brightness of 494 mJy/beam (Venturi et al. ...

MICROSCOPES . ... In the last three to five years, LOMO has developed new lines of products, including new families of biological, fluorescent, and polarizing microscopes, night vision devices, consumer Maksutov telescopes, etc. ... 1939 Company introduces its first student and biological microscopes. as well as its first manual movie camera . ... 1956 LOMO produces its first wide-screen-format movie projector and introduces its first fluorescent microscope for chemical structure analysis. ...

NMW survey overview . Access image archive . ... The New Milky Way survey aims to detect bright (V<13.5) optical transients near the Galactic plane using an automated wide-field (8x6 deg.) system capable of surveying the whole Milky Way area visible from the observing site in one night. ... All images obtained during the transient search survey are available online (please use the image archive access form ). ... Images per field: . ... Images per night: . ... Milky Way imaging time: . ...

... 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 . ...

Russian Version ( KOI-8 , Win ) . Institute of Astronomy of the RAS . ... Self-consistent simulation of chemical and dynamical evolution of protostellar clouds . Chemical evolution of galaxies . ... Soon after my birth I was moved (I was not able to move on my own in those times, you know) in Novouljanovsk, small town to the south of Uljanovsk. ... Since that time my life and work is bound to the Institute of Astronomy of the Russian Academy of Sciences. ... Back to the INASAN home page . ...

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Астрономия и Космос Небесные тела Черные дыры и пульсары . А строномы получили наблюдательные подтверждения того, что некоторые черные дыры вращаются вокруг своей оси , подобно водоворотам. ... Следовательно, черные дыры , как и нейтронные звезды, могут вращаться вокруг своей оси . ... Комментарии к Черные дыры вращаются вокруг своей оси . Ссылки по теме Черные дыры вращаются вокруг своей оси: . Черные дыры вращаются вокруг своей оси . Черные дыры и пульсары . Имитация черных дыр . ...

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