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21. Galaxy Group HCG 87
Astronomy Picture of the Day . Galaxy Group HCG 87 . ... The large edge-on spiral near picture center, the fuzzy elliptical galaxy immediately to its right, and the spiral near the top of the image are identified members of the group, while the small spiral galaxy in the middle is likely a more distant background galaxy. ... While not exactly locked in a group hug , the HCG 87 galaxies are interacting gravitationally, influencing their fellow group members' structure and evolution. ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/1207263 -- 14.3 Кб -- 18.07.2005
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22. Mees Observatory
... ASRAS HOME . Radio Astronomy . ... About ASRAS . ... Our Observing Site . ... 2015 Mees Tour Guides . ... We're offering Regular Tours (a presentation on astronomy geared to a general audience, followed by a tour of the observatory and (hopefully!) observing of several objects, which may include the Moon, planets, nebulae, star clusters and perhaps galaxies), and Kids' Tours (a more interactive presentation specially aimed at youngsters plus the observatory tour and observing) as in prior years. ...
[ Сохраненная копия ]  Ссылки http://www.rochesterastronomy.org/Mees-Observatory -- 34.0 Кб -- 09.04.2016
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23. Yaroslav S. Yatskiv
... Dept. for Astrometry & Space Geodynamics . ... Dept. for Physics of Stars&Galaxies . Dept. for Space Plasma Physics . Dept. for Physics of Minor Celestial Bodies . Dept. for Physics of Planetary Systems . Dept. for Solar Physics . ... History of MAO . ... NAS of Ukraine . ... 2016,MNRAS, 2016MNRAS.tmp.. ... Geodynamics: application of space geodesy techniques for geodynamics . ... Head of the Space Geodynamics Department of MAO (1979 - ) . ... Prof. Yaroslav S. Yatskiv . ... MAO NASU . ...
[ Сохраненная копия ]  Ссылки http://www.mao.kiev.ua/index.php/en/databases/67-person/128-yasyatskiv -- 18.8 Кб -- 10.04.2016
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24. ADASS Conference Series
... He joined ESO in 1990, to integrate the Image Processing Group for the development of instrument-related software in MIDAS. ... Carlos is a staff member of the European Space Agency, currently working in the XMM-Newton Space Operations Centre, at the European Space Astronomy Centre (ESAC), located in Villafranca del Castillo, Spain. ... He is currently an associate professor at the Astronomy Data Center (ADC) of the National Astronomical Observatory of Japan in charge of data management. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/POC.html -- 17.0 Кб -- 04.04.2016
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25. http://lnfm1.sai.msu.ru/~math/docs/abs_ngc80.pdf
The Chemically Distinct Nucleus and Structure of the S0 Galaxy NGC 80 O. K. Sil'chenko1, S. E. Koposov1, V. V. Vlasyuk2, and O. I. Spiridonova 1 2 2 Sternberg Astronomical Institute, Universitetski i pr. ... The global stellar disk of NGC 80 has a two-tiered structure: its outer part has an exponential scale length of 11 kpc and normal surface density, while the inner disk, which is also exponential and axisymmetric, is more compact and brighter. ...
[ Текст ]  Ссылки http://lnfm1.sai.msu.ru/~math/docs/abs_ngc80.pdf -- 218.7 Кб -- 06.03.2003
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26. INTERNATIONAL CONFERENCE ON SCIENCE AND TECHNOLOGY PROBLEMS AND PROSPECT OF THE
... Events INTERNATIONAL CONFERENCE ON SCIENCE AND TECHNOLOGY PROBLEMS AND PROSPECT OF THE PROPULSION ENGINEERING DEVELOPMENT . ... INTERNATIONAL CONFERENCE ON SCIENCE AND TECHNOLOGY PROBLEMS AND PROSPECT OF THE PROPULSION ENGINEERING DEVELOPMENT . ... Development prospects and use of engines for aviation, space - rocket systems, motor transport mechanical engineering and stationary power supply installations . ... Propulsion engineering, power engineering and space vehicle ecology problems . ...
[ Сохраненная копия ]  Ссылки http://www.ssau.ru/engevents/show/?id=613 -- 27.2 Кб -- 19.02.2016
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27. NICMOS Imaging of QSO Host Galaxies at 0.1 < z < 4.4
... We present preliminary results from two programs to image the host galaxies of radio-quiet quasars in 1.6 micron light using NICMOS camera 2 on HST. The high redshift program consists of QSOs covering the redshift range 0.8 < z < 4.4 and a range of QSO luminosities. Of the six objects for which data have been obtained the results range from no host galaxy detected, to an obvious galaxy with an interacting companion, to a possible high