... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... Brief History of Rocket and Space Technology . ... ISS Russian Segment . ... Sea Launch . ... News . ... OAO RSC Energia is a leading enterprise of rocket-space industry, the prime organization for manned space systems. ... Contribution of RSC Energia to the Russian Rocket-Space Technology . ... RSC Energia: Progress MS-02 docked with the ISS.' ... 2015 JSC "S.P. Korolev RSC "Energia" . ...

... 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 . ...

The Database of Close Binary Systems . ... Team . ... This web-based interactive database is being developed and maintained by a team at the Sternberg Astronomical Institute of the Moscow State University . The project is an on-line extension of our catalogue on "Highly Evolved Close Binary Stars" (volumes I, II) published by Gordon and Breach in 1996. As of September 2009, the database (both the software and the content) is in its development/testing phase. ...

... A new approach to the object-oriented logic programming of Internet agents is introduced. ... These methods are based on the technique of modifiable reasoning in the dynamic Internet environment and on the Actor Prolog object-oriented logic language that we developed. ... Class instances in Actor Prolog are constructed implicitly as Vol. ... We developed a logic object-oriented model of asynchronous computations for programming the multiagent logic systems and implemented this model in Actor Prolog....

... Regular changes of the large-scale CGLB distribution in dependence on the phase in the solar cycle are presented. ... 9.02.76 - 20.07.76 90 45 0 -45 -90 0 90 45 0 -45 -90 0 60 120 180 240 300 360 0 60 120 180 240 300 360 0 20.04.77 - 30.09.77 7.05.78 - 16.10.78 90 45 0 -45 60 120 180 240 300 360 0 -90 60 120 180 240 300 360 30.03.79 - 9.09.79 25.06.81 - 5.12.81 22.09.83 - 4.02.84 90 45 0 -45 60 120 180 240 300 360 0 -90 60 120 180 240 300 360 Figure 1. ... Here, the CGLB is extremely low. ...

. Variable stars - are characterised by the changeable glifter. There are eclipse twin stars and pulsing variable stars (cepheids) with the periodical changing of a glifter, eruptive stars, pulsars and closed twice stars. Back .

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . des actualitГїs . ... les plus belles images de l'Univers dГїcryptГїes pour vous . ... des pages consacrГїes Г la publication de vos photos Mais c'est aussi une vraie communautГї avec laquelle partager votre passion et nourrir votre curiositГї. Accueil Г? la une Le ciel change . ... L'espace, une vigie pour la biosphГЕre . ... 20/01/2015 - Une multitude d'Гїtoiles hors des galaxies . ...

... 2006 . ... Comparison of total ozone distribution in the high latitudes of both hemispheres SCAR XXIX Open Science Conference, 2006, 12-14 July, Hobart, Australia - Abstract Volume. ... Analyses of spectra, stability and eigenmode transverse small-scale oscillations in the inner Earth magnetosphere. 6th Open Conference of Space Projects Evpatoriya, September 2006, Abstracts . ... Ps6 pulsations in the Earth magnetosphere. 5th Open Conference of Space Projects Evpatoriya, September 2005, Abstracts . ...

. Christmas History Traditions Carols Celebration in UK Celebration in USA яhristmas Menu .

. Prague, August 16, 2006 . Present classification : Suggested: . E, EA, EB, EW, EP E, EA, EC - contact (merging EB and EW), EP PN, WD, WR Remove from the classification, indicate through the spectral type or Remarks RS If such a star has eclipses, give notation like EA+RS, RS+EA . AR, D, DM, DS, DW, K, Remove from the classification; KE, KW, SD as a rule, these types in the GCVS are based on indirect evidence . ECLIPSING VARIABLES . (the description of the class should not mention close binarity)

This section of library contains information about "classic" Star Catalogs. ... For a Henry Draper Catalog 272149 stars have received a total of 531,211 identifications in 7 сatalogs: . 270456 - in Astrographic Catalogue ( "Carte du Ciel", 4M), . 251943 - in Guide Stars Catalog (GSC), . ... A file with information on the components of 1788 of multiple systems in catalog HDEC (3681 component, or a combination thereof, with 4054 recording). ... A file with information about 21971 variable stars. ...

АНОНС НАУЧНЫХ КОНФЕРЕНЦИЙ 1998-99 гг. ... An AAS Electronic Announcement Dear Colleague: NASA has approved development of a Wide Field Camera 3 (WFC3) for installation in the HST on the 2002 Servicing Mission. A Scientific Oversight Committee (SOC) is being established to ensure that the broad interests of the scientific community are represented in the development of WFC3. The primary task of the SOC will be to advise the HST Project and STScI in all areas of scientific performance of WFC3. ...

Previous Editions of the M111: . ... OutReach Training and Program . September Public Night . Welcome all ye weary travelers to a new type of M111 "On Line". ... Back to top.. ... When I logged our last outreach programs I couldn't help but notice that Warren Rupp Observatory is NUMBER FIVE in the worldwide standings in public outreach programs! ... If you'd like to train in astronomy outreach, just contact any of our members and we'll be happy to train you to do public outreach! ...

Institute of Nuclear Physics Russian Akademy of Sciences BAKSAN (KABARDINO-BALKARIYA,tower ELBRUS), RUSSIA BAKSAN ( BKSN ), 6 NM64 NEUTRON MONITOR (REMOVED FROM NLC2) CORRECTED FOR PRESSURE Altitude 1700 M Mean= 4708.4 May 2007 Geographic Coordinates ... (1965)= 5.6 GV; SF= 100 Pressure Coefficient= -0.73 %/mb Corrected to 820 mb Standard Pressure Comment: 1.000 4706 4704 4696 4682 4699 4705 4711 4727 4714 4705 4707 4733 4705 4722 4727 4721 4702 4703 4707 4703 4703 4693 4684 ...

... The source exhibits a mas-scale structure which, according to the USNO multi-epoch monitoring at 2.3 and 8.4 GHz over the period from 1994 July through 1998 April, undergoes considerable changes in the brightness distribution and positions of the major structural features. Our image is qualitatively consistent with the structural pattern of the source. ... We note a difference of ~90 in position angles of secondary components in our image and the 5 GHz VLBI image by Shen et al. 1998). ...

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