... Denis Puy . ... More recently, Puy & Signore (1995), from this simple description, but with a more complete chemistry (primordial , HD and LiH molecules) considered the three phases of the protoclouds supposed to be initially spherical: i) a linear evolution which approximately follows the expansion, ii) a turn around epoch ( ) when the protocloud reaches its maximum value, and iii) a non-linear evolution or the collapse of the protocloud. ... Puy D. et al. ... Puy D. 1996, A&A, in press . ...

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• Ionization and Thermal Structures of the Absorption-Line Systems of Quasars
• Star formation rates from young-star counts and the structure of the ISM across
• HST this week: 057

... Next: The PROS Big Up: Software Systems Previous: Data Reduction Software . ... The srcinten task provides PROS users with a tool to compute count rates for point sources in the ROSAT High Resolution Imager (HRI). ... Corrected upper limits are cited at locations where the count rate falls below the source detection threshold. ... Srcinten is a new PROS task that computes and applies the above correction factors to the net counts in a user-specified aperture. ...

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• Spatial Structure of NGC 6822: An Example for Statistical Modeling of
• Propagating Uncertainties and Units in Data Structures
• A Generic Data Exchange Scheme Between FITS Format and C Structures

... Research . ... The aim of this project is to study the nearest spiral galaxies in the nearby Sculptor Group in neutral hydrogen with the ATCA to search for high-velocity clouds (HVCs) and extra-planar gas in their environment. ... The Sculptor Group is the nearest galaxy group. ... Therefore, we have mapped a large area of almost $2^{\circ} \times 2^{\circ}$ around the two nearest large Sculptor Group galaxies, NGC 55 and NGC 300, with the ATCA in mosaicking mode. ...

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• Neutral hydrogen absorption

. ___________________________________________________________________ The Electronic Universe Project e-mail: nuts@moo.uoregon.edu

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• Astronomy Plus CCD Images of Galaxies
• The Galaxy Gallery: Messier Objects
• Formation of the Earth's Moon

Below is the sample image and caption given out at the AAS meeting. ... Dark, sinuous clouds of cold hydrogen gas reveal themselves as shadows against the glow of warmer, brighter clouds in the background. ... This image, made with radio telescopes at the Dominion Radio Astrophysical Observatory near Penticton, British Columbia, was presented to the American Astronomical Society meeting in Austin, TX on January 8, 1999. PHOTO CREDIT: Steven Gibson and Russ Taylor of the University of Calgary. ...

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• HISA Poster for the 195th Meeting of the AAS, January, 2000
• Heiles Symposium Presentations
• Galactic Spiral Structure in H I Emission and Self-Absorption

This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

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... Another significant contribution to the crystal energy of metals is the electron-ion interaction or the electron bandstructure energy (E BS ) which is defined by the interaction of valence electrons and the Brillouin zone (BZ) planes. ... The program BRIZ has been developed for 3D visualization of Brillouin zone configurations and intersections of BZ planes with a Fermi sphere[4]. ... 1.75 (electrons/atom). ... 4] Degtyareva V.F., Smirnova I.S.: BRIZ: a vizualization program for Brillouin zone ? ...

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• Grants LSR ISSP RAS
• Laboratory of spectroscopy of defect structures ISSP RAS
• LHPP ISSP RAS

... Mokhovaya st., 11, Moscow, 103907, Russia. ... July 15-17, 1999 , pp. 161-164 . A method for multiple access using the structure of the unstable periodic orbits of chaotic attractor is proposed. Possible principles of the control and selection of unstable cycle-codes are presented. ...

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• Project 8 - RFBR - Development of novel superconducting oxide electronic
• Chaotic Processors and Unstructured Data Bases - NDCS-99
• IRE RAS Laboratory of Electromagnetism

... The HH flow associated with young stellar object HL Tau has an exciting history and even until now the origin of some its features is not clear yet. ... Knotty structures of Herbig-Haro jets are common phenomena and knowing the origin of such structures is essential for understanding the processes of jet formation. ... In the flow detected compact knots with high (-150 km/s) and bow shape structures in front of those, with low radial velocities (-50 km/s). ...

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• V1494
• New data on the cpmplex field structure of chemically peculiar stars

Databases (NSDC) of the Natural Planetary Satellites. ... NSDC: Database of astrometric observations of Natural Planetary Satellites . ... They are thoroughly looking for observations in different sources, creating their owndatabases which are then mostly inaccessible to other researchers. ... In the file "content" with explications, the reference is given to the data source as well as the bibliographic reference. ... Data sources. ... Why a specific bibliographic database for Natural satellites? ...

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"Dynamical friction and formation of structures: some cosmological aspects", Astroph. Space Sci., v.123, p.393-402, 1986 (with S.G.Simakov). "Accretion Mechanism of the Formation of Large Scale Structure of the Universe", Astron.Zh., vol.66, p225-231, 1989 (with S.G.Simakov). Back .

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• Structure of the Galaxy
• Calculation of binary NS coalescence rates

... Science . ... Science Users Information > Science Activities > Science in Garching . ... Observing with ESO Telescopes . ... Data Handling and Products . ... Understanding the diversity and consequences of star and planet formation is a key area of research for ESO. ... Read more and see who is involved in this research area.. Stellar structure and evolution includes the internal structureof stars, the structure and dynamics of stellar atmospheres,as well as stellar winds and mass-loss. ... ESO . ...

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• ESO - Research Area: STELLAR STRUCTURE AND EVOLUTION
• pyQC: script structure
• ESO - PhD Thesis Topics offered by ESO Faculty Members

. Language [RU/EN] Search: . Home . UP . Research . Projects . Services . Info . News . Events . Personal . Archive . Ionosphere and radiowave propagation: structure . The main page . Information . Publications: . 2011 - 2015 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2000 - 2004 . 1995 - 1999 . Participation in International symposiums and conferences: . 2013 - 2015 . 2011 - 2012 . 2009 - 2010 . 2007 - 2008 . 2005 - 2006 . 2002 - 2004 . N.V. Pushkov . 09/04/2016 23:52 MSK . webmaster@izmiran.ru .

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• ON THE STRUCTURE OF 3.11.94 ECLIPSE CORONA
• Information
• Ionospheric database formation

... The main research task of the LRS was an investigation of interstellar medium of our Galaxy using its line emission in radio domain with the help of the gratest RATAN-600 Radio Telescope. ... The complex investigation of the Interstellar Clouds structure on the different scales and with the different radio lines for understanding of structure, dynamics and evolution of interstar gas and its interaction with other galactic constituents and the conditions for star formation. ...

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• Laboratory of spectroscopy and photometry of extragalactic objects : Vortex1
• Results scientific researchs 12

Scale-heights of the Galactic disk subsytems with different ages and metallicities . V.Marsakov & Yu. ... It is based on the fact, that all stars cross the disk plane several times during their Galactic orbital period. ... We have used our representative sample of nearby disk F2-G2 stars Marsakov & Shevelev (1995) in which fundamental stellar parameters was determined on the basis of published date on uvby-photometry, proper motion and radial velocities. ... Marsakov V.A., Shevelev Yu.G. Bull. ...

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• Vladimir Marsakov Abstracts
• Vertical Structure, figures

... Using the spectra was taken with 4m telescope of the Kitt-Peak observatory (USA), on the basis of a new method of stellar population determination, which combines advantages of both evolutionary and population syntheses, a study of the stellar population and evolutionary characteristics - metallicity, age and mass function was carried out for the Blue Compact Galaxy (BCG) SBS~1331+493 with low heavy element abundance, undergoing the burst of star formation. ... Arrows show the regions. ...

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• Andrew Ugryumov's "Structure" Home Page
• Pustilnik Simon's "Structure" Home Page
• Pramsky's home page Pramsky Alexander's "Structure" Home Page

Back to Martin Elvis' Home Page . Color 2-D figure of structure (postscript) . 3-D views of the quasar structure: . 3-D Top view 3-D End-on view 3-D Side view . ... Quasar Atmospheres: Toward a `Low' Theory of Quasars , (Elvis M. 2003 astro-ph/0311436 , to be published in AGN and the SDSS, eds. G. Richards and P. Hall) . Talk from the Leicester `Winds Tori' Workshop, Sept 2004 (pdf, 21 pages) . Disk Winds summary from the Leicester `Winds Tori' Workshop, Sept 2004 (pdf, 7 pages) . ...

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• Model Spectra for Spectral-Fitting Program
• The AstroStat Slog Blog Archive Differential Emission Measure [Eqn]
• Vertical Structure of the Secondary: Hydrostatic Model

... General information . ... Staff . Research staff . Technical, administrative & librarian staff . ... Research . ... Infrared astronomy . ... Solar physics . ... Library . ... Friends of Arcetri . ... Computing Science . ... Operating Systems and Languages . ... General Physics . ... Structure of the Matter, Atomic and Nuclear Physics :General interest texts . ... Plasma Physics : General interest texts . ... Astronomy : General interest texts . ... Physics of the Planetary System . ...

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• Arcetri Star-Formation Group Publications
• Deadlines - IGM@50: Is the Intergalactic Medium driving Star Formation? - June
• Guidetta Torricelli

... IAU planet classification Observing with a Telescope Large Scale Structure The observables: Local Group (size 1 Mpc) Virgo cluster (size 2+ Mpc) Virgo supercluster (size ~33 Mpc) Voids (size ~ 10-150 Mpc), Walls and sheets, aka filaments (size ~ 50-80+ Mpc) 1 parsec The nearest star is 1.2 parsecs away (Proxima Centuri). ... Virgo supercluster Voids, Sheets Filaments The Virgo Cluster is a cluster of galaxies at a distance of about 18.0 Mpc away in the constellation Virgo. ...

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• http://www.aaa.org/s932/images/09fallclass3.pdf
• http://www.aaa.org/s932/images/09fallclass2.pdf

... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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• Extragalactic Astronomy
• Olga P. Verkhoglyadova
• Stellar Astronomy