... Laboratory for Spectroscopy of Molecular Structures . ... Staff . ... Doctor of Sciences, Head of the Laboratory . room 315 . phone No. 2-84-65 . ... Doctor of Sciences, Leading Research Associate . room 308 . ... Candidate of Sciences, Senior Research Associate . room 329 . ... 2-84-65 . ...

... The analysis shows, that asteroid ­ rubble pile loses its fast fragments in no time but the retaining fragments forms a compact structure immersed in dust ­ gas atmosphere, created by interaction of interplanetary medium with dispersed product of collisional evolution of asteroid. By interaction of an asteroid ­ rubble pile with interplanetary medium structures asteroid can increase its brightness on account of blowed up dust simulating phenomenon of distant comet's brightening. ...

True Color Image Gallery: Galactic SNR | Magellanic Cloud SNR . ... Radio Images Page . ... Exposure uf . ... 10102 . ... Exposure uf Exposure time of unfiltered event file . Exposure f Exposure time of filtered event file . ... Click left mouse button on hyperlink below to download file . ... Event 2 FITS File . ... AUX file . ... see fit detail page for more about the fit. see chandra spectrum page for region used. Images in Several Energy Bands . True Color Image . ... 1.0" . ...

... Recall that (Voevodsky's) motives correspond to a certain 'universal cohomology theory for smooth algebraic varieties'. Note that in contrast with 'classical' categories of motives (i.e. Chow, homological and ef numerical ones) Voevodsky's DMgmf DMgm are endowed with natural (and highly non-trivial) structures of triangulated categories. ... I also proved several new results on motives: they concern coniveau spectral sequences, motivic cohomology, and unramified cohomology. ...

Large-scale wave processes in space plasma. ... G.V.Lizunov, O.P. Verkhoglyadova, and K.I. Churyumov, Plasma- beam instabilities in comatary ionospheres, Russian Astronomical Journ. ... Verkhoglyadova, O.P., V.V. Grimalsky, Propagation of ion- sound solitons in unhomogeneous plasma, Ukrainian Phys. Journ., ... Verkhoglyadova, O.P., Ivchenko, V.N., Plasma regime identification technique using magnetospheric satellite measurements, Space Sci. and Technology, 4 (5/6), 18-27 (1998) (in Ukrainian). ...

... 12 Oct 02 2006 1.9 Jan 26 2006 8 CB,CS,R=F. R=G, SMALL, TIGHT, BRIGHT NGC 1912 M38 17mmAT 2012 M.M . Open Cluster 8.0 II 2 r CL,B,VL,VRI,IF,STL$S Mar 16 2012 18 Mar 01 2011 12 Mar 08 2010 12 Dec 16 2009 12 Mar 20 2009 16 Mar 17 2007 1.9 17mmAT M.M . 2011 - MANUAL SETTING CIRCLES M.M . 2010 MANUAL SETTING CIRCLES 26mm 20mmUW MESSIER MARATHON - 2009 26mm ...

... Its perihelion would occur on April 1, 1997, at which point the comet would be only 0.92 astronomical units from the Sun, just within the orbit of Earth. ... Taken in April 1993, the photo showed the comet over 13 astronomical units from the Sun, well beyond the orbit of Saturn. ... Hale, as in Comet Hale-Bopp, has written a book, Everybody's Comet (available through the ASP Catalog) and coordinated an Internet project, "Hale-Bopp: Live in the American Classroom." ... Anatomy of a comet. ...

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

... Magnetic Storms . ... Cosmic Rays . ... Energetic Particles . ... Solar fast Particles . We cannot observe the way the distant universe accelerates cosmic rays or produces energetic photons, but acceleration processes also occur on our Sun , though on a much more moderate scale. ... That is why such events are often missed by cosmic ray detectors near the equator, where the lowest energies are excluded by the Earth's magnetic field. ... Should we be concerned about solar energetic radiation? ...

You Can Make Stellar Images Brighter . Articles | ... A few months ago I wrote an article titled "You Can’t Make Them Brighter". So why am I now writing that you can make them brighter. ... The image of a focused star is actually a small disk called the Airy disk, named after the 19 th century scientist Sir George Airy. ... For a given aperture, a smaller Airy disk means that the light is focused to a smaller disk and is therefore brighter. ... www.astronomy.net . About Astronomy Net | ...

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. ...

... QUALITY FLAGS Each source has an associated ``quality flag''. ... 0 1 Source lies above one or more bad pixels . ... 5 32 Source lies within central enhanced region . ... For example, a source with a bad pixel and lying on or close to a read-out streak would have bits 0 and 1 set and thus have a quality flag of 3. QFLAG The quality flag for each source in each filter obtained from the input source-lists. ... 0 1 Point source has one or more sources within a radius of 6-12 unbinned pixels . ...

. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

... Our Galaxy . ... Stars . ... Spiral arms are home to much more than just the brightest stars, however. ... Spread along the bright spiral arms can be seen prominent dark lanes, clouds of molecular gas and dust which obscure the visible light. ... The spiral arms are lit up by the extraordinary luminous young massive stars that are born within the dark clouds of molecular gas that lie along the arms. ... This interpretation тАУ of a spiral galaxy with active star formation within it тАУ is not...

Influence of dust on the galactic structure Dust distribution models Influence of dust on the galactic structure Dust distribution models Dust in galaxies The effects of absorbing material in galaxies were recognized before the physical nature of galaxies became clear. ... Influence of dust on the galactic structure Dust distribution models Influence of dust on the galactic structure Dust distribution models For instance, = 5 = A = 5.m 4 (screen), A = 1.m 75 (slab). ... Real galaxies ­ Cµ 0.5. ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... Company's History . ... History . ... Graduated from Moscow Aviation Institute (1941), Doctor of Science, Engineering (1957), professor, corresponding member (1958), full member (1966) of ... Sciences, of the International Academy of Astronautics. 1932 to 1934 - apprentice mechanic at factory apprenticeship school of TsAGI, Moscow . 1934 to 1935 - mechanic at Special Tasks Shop of TsAGI, Moscow . 1940 to 1941 - designer at Plant 84, Khimki...

ATMoB "Galaxy Observing Award " Guidelines Purpose: To promote observing among the membership of the Amateur Telescope Makers of Boston through participation in the Galaxy Observing Awards program. ... Examples of elliptical galaxies: M49, M59, M60, M87, NGC 4125. Limiting Magnitude Assessment: Spirals: A spiral galaxy consists of a flattened disk, with stars forming a (usually two-armed) spiral structure, and a central concentration of stars known as the bulge. ...

... 110, A09S07, doi:10.1029/2004JA010931, 2005 CORONAS-F/SPIRIT EUV observations of October ­ November 2003 solar eruptive events in combination with SOHO/EIT data V. V. Grechnev,1 I. M. Chertok,2 V. A. Slemzin,3 S. V. Kuzin,3 A. P. Ignat'ev,3 A. A. Pertsov,3 I. A. Zhitnik,3 J.-P. Delaboudinie e,4 and F. Auche e4 `r `r Received 30 November 2004; revised 2 March 2005; accepted 8 April 2005; published 28 July 2005. ... Events of the First Rotation 3.1. ... SPIRIT AND EIT OBSERVATIONS A09S07 Figure 1. ...

... Imaging of the core of the OMC-1 region using NICMOS camera 2 through the F212N and F215N filters shows a wide variety of interesting structure on scales of 0.2" at a very high dynamic range (Stolovy et al. ... The application of image restoration techniques, including multi-channel variants of the Richardson-Lucy technique, offers the chance to enhance structure on the finest scales and also to suppress the prominent and richly structured point-spread functions of the many bright stars in the...

... CNRS - RAS RFBR Associated European Laboratory "Physical Properties of Coherent Electronic States in Condensed Matter" between Institut Neel, CNRS and Kotel'nikov IRE RAS (2008-now), member . ISTC, Elements for Micro- and Nanoelectromechanics Based on the Whiskers of Quasi One-Dimensional Conductors and HTSCs (2006-2009), participation . ... RFBR, Electron and spin transport in low-dimensional structures (2013-2015) . ... RFBR, Conduction and energy states of chain structures (2010-2012) . ...