. January 2000.01 . February 2000.02 . March 2000.03 . April 2000.04 . May 2000.05 . June 2000.06 . July 2000.07 . August 2000.08 . September 2000.09 . October 2000.10 . November 2000.11 . December 2000.12 . часть a . часть b . часть c . часть d . Musical Kp diagram 2000 (*.pdf)

To see a Russian version of this page, click here . ... Graduated from Moscow State University (MSU), Faculty of Physics in 1976. Ph.D. degree - 1988, MSU. Main field of scientific activities: photometric investigations of various stars, close binary stellar systems and other astronomical objects, including research with use of fast photoelectric photometry with a high time resolution till 1 millisecond. ... New portable photometer . ... Send your mail to: tem@sai.msu.ru ...

... Camera (cold) going up to observing level for insertion into Telescope using the handling tool (blue). July 2007 . image: VISTA_IR_Camera_to_Telescope_2.JPG . ... Camera being moved from its stand in the lower floor of the Enclosure below the Azimuth floor, using the handling tool (blue). image: remove camera from stand.jpg . ... Camera inside the upper part of the enclosure after being lifted up to the Azimuth floor on its handling tool (blue). image: camera reaches az floor.jpg . ...

... Measurement of the MASS detectors parameters with mass program January 24, 2015 [112707] . MASS/DIMM electronics. ... Turbina-core(D): Dimm User Guide. ... N.Shatsky, V.Kornilov, The revision of the MASS/DIMM star catalogue. ... О.Возякова, В.Корнилов, Н.Шатский, Новое программное обеспечение прибора MASS/DIMM. ... V.Kornilov, N.Shatsky, S.Potanin, O.Voziakova, B.Safonov Preliminary results of astroclimate parameters measurements at the Sternberg 2.5m telescope installation site. ...

... М15: плотное шаровое звездное скопление . ... Hubble Heritage Team ( STScI / AURA ), NASA . ... Находящееся всего лишь в 40000 световых лет от Земли в созвездии Пегаса скопление M15 является одним из наиболее плотных шаровых звездных скоплений в нашей Галактике. В каталогах скопление M15 также обозначают NGC 7078) Это великолепное изображение, полученное космическим телесокопом им. Хаббла, позволяет увидеть тысячи отдельных звезд в центральной части скопления размером порядка 10 световых лет. ...

. Эволюция массивной звезды . Хмический состав звезды с массой в начале горения углерода . Зависимость плотности вещества в центре звезды от температуры, показывающая эволюцию звезды с массой . Указаны времена выгорания различных элементов и нейтринная светимость звезды . Ядерные реакции, приводящие к синтезу элементов от гелия до германия. All Your comments, suggestions and bug reports (any kind) are welcome here . Last updated 13 April 1997 year.

... The length of the module is 13.0 m; maximum diameter 4.3 m; mass at the launch 19000 kg. Module Priroda was launched from Baikonur on April 23, 1996 by the LV Proton-K. It docked to the nose docking port of the core vehicle and by its robot arm redocked to the side port. It is the newest module in the OC. ... The composition of the scientific equipment of the module is given below. Дизайн и поддержка CosmoWorld.ru, 2001 . ...

Habble cosmic telescope. ... It became possible to study all occurrences on Mars (for example the season changings of the polar "hat" of Mars), on Jupiter satellites, ets. ... The scientists saw the details of the galaxy gas nebulas, the most dense central parts of the ball star congestions and galaxies to proof the existance in the cores of many galaxies invisible objects with the mass of hundred millions and milliards of the Sun's mass (evidently black holes). ...

... The source exhibits a mas-scale structure which, according to the USNO multi-epoch monitoring at 2.3 and