. F IGURE . 1. The distribution of F stars in our sample from the observed distances from the Sun. Solid curve gives a power-law approximation of the number of stars as a function of the distance within R obs =50 pc and the dashed line is its extrapolation up to 60 pc. The arrow indicates the upper boundary of the domain where the sample is complete. discussion in the text | next figure .

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• DocladVertical Structure, figures

... The International Conference "Mode Conversion, Coherent Structures and Turbulence" will be held in the Space Research Institute of RAS during the period from 23 up to 25 November 2009. ... The international conference MSS-09 is organized by Space Research Institute with participation of the Russian Academy of Sciences, the Dynasty Foundation, the Russian foundation of fundamental researches, the European Geosciences Union, the Education and the Scientific Council on Nonlinear Dynamics of RAS. ...

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• Substorm fine structure [Oulu]
• Attitude file structure
• List of currently available KP AZ.

... Output: ; The specified disk file is created or modified. See also: ; modech, rdech, wdech ; ;History: ; 27-Jul-1998 Valenti Initial coding. if n_params() lt 2 then begin print, 'syntax: wdech_ raw , ech , file (. ech assumed)' return endif ;Make sure input data are in a structure . sz = size( ech ) ;variable info block if sz(sz(0)+1) ne 8 then begin ; true : not a structure message, /cont, 'spectrum data must be a structure - aborting' return endif ;Make sure input ...

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• The Opacity of Spiral Galaxy Disks. VIII. Structure of the Cold ISM
• Superconducting Confined Electron Devices for Possible Application as
• File and Table Structures

... Because of the low conductivity, the magnetic coupling is weak and depends critically on density, temperature, ionisation rate and charged species. ... Implications When the Hall regime dominates near the midplane and ambipolar diffusion is dominant closer to the surface, a thicker layer of the disc is unstable to MRI perturbations and modes grow faster than under the ambipolar diffusion approximation. ... Right panel: For weak coupling, Hall limit perturbations grow until vA/cs ~ 2.9. ...

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• Vertical cross-section of an A9 main sequence star
• Telescope structure
• Assembling the telescope structure

The cosmic microwave background, shown at left in this illustration, is a flash of light that occurred when the young universe cooled enough for electrons and protons to form the first atoms. ... The universe then went dark for hundreds of millions of years until the first stars shone and the first black holes began accreting gas. A portion of the infrared and X-ray signals from these sources is preserved in the cosmic infrared background (CIB) and its X-ray equivalent, the CXB. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7B38E7BC69-5958-4E1B-8887-DA5F5EC6DD63%7D
• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BE07E3F4E-BB21-4972-BB19-80E5506D99AD%7D
• Mini-halos began cosmic structure | Astronomy.com

... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Properties of kinematically decoupled structures in Early-Type Galaxies . ... Science Users Information . ... ESO-MIDAS . ... ESO Science Newsletter . ... The project consists in measuring the stellar kinematics, stellar populations, dynamics, and morphological properties of the kinematically decoupled structures observed in the inner regions of Early-Type Galaxies. ... Return to list of thesis topics...

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• ESO - Joint ESO MPA MPE TUM Excellence Cluster Universe Conference: Theoretical
• COBRA file structure
• CHAMELEON file structure

The CHIANTI database consists of 4 primary ASCII files for each ion in the database. contains the energy levels in cm^(-1) It includes both experimental data and theoretical values of the levels energies. ... For consistency with Griffin et al 2000, who adapted their atomic structure calculation to a set of observed energies identical to the NIST one, we use the NIST v.2 level ordering. %produced as part of the Arcetri/Cambridge/NRL 'CHIANTI' atomic data base collaboration % % E.Landi - Nov 2004 . ...

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• APOD: February 7, 1998 - COBE Hotspots: The Oldest Structures Known
• Kernel Configuration and Makefile Structure
• Ray Structure - Halley's Comet

... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Universitetsky 13, Moscow 119899, Russia, shev@sai.msu.ru . ... 1.Sternberg State Astronomical Institute, 119899, Moscow, Russia. shev@sai.msu.ru . ... V.V.Shevchenko, Sternberg State Astronomical Institute, Moscow University, Moscow 119992, Russia, shev@sai.msu.ru . ... 119992 Moscow, Russia; . ... 2Sternberg Astronomical Institute, Moscow University, Moscow, 119992, Russia, . ... Moscow, 119992, Russia shev@sai.msu.ru . ...

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• Пугачева Светлана Георгиевна

. Graca Rocha - Research . For a summary I'm interested in the study of the Cosmic Microwave Background Radiation Temperature and Polarization Anisotropies, non-Gaussianity, Topology of the Universe, Varying Fundamental Constants Theories, Weak Lensing, Large Scale Structure, etc.. Last updated: 2005 June. home .

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• OptInt PmWiki : Wiki Structure
• OptInt PmWiki : Wiki Structure | Attach
• A varying fine structure constant, alpha

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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• Y.Kupryakov, SAI, MSU
• Data base of Natural Satellites. Documentation. Structure

"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
• Seminars
• PROBLEMS OF THEORETICAL COSMOLOGY - UISS2000

... First of all I would like to mention about the vanishing cohomology associated to the Milnor fibre of the isolated hypersurface singularity. We review the results on the Milnor number (local and global) by Kouchnirenko (Inventiones math. 32, No1 (1976), 1-32) and then roughly sketch the formula of Hodge numbers given by Danilov (FAA, 13, No.2(1979),32-47). ... The Hodge structure of the cohomology of an affine hypersurface in an algebraic torus will be discussed. ...

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• Hamiltonian structures and evolution equations (Fall 2001)
• Conference "Combinatorial Methods in Physics and Knot Theory" (February 2005)
• Differential geometric structures (Spring 2002)

... Structure of Data . ... Catalog . ... Catalog: 206 clusters 32 clusters: known before 12 clusters: parameters from BVRI photometry @ SAO 1-m 0 clusters: parameters from UBVRI photometry @ Maidanak 1.5-m 26 clusters: parameters from 2MASS 168 clusters: new (2MASS) 142 clusters: parameters from 2MASS 26 clusters: embedded 0 clusters: parameters from BVRI photometry @ SAO 1-m 3 clusters: parameters from UBVI photometry @ ARIES 1.04-m 0 clusters: parameters from UBVRI photometry @ Maidanak 1.5-m . ...

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... Number of trailing spiral waves of surface density is equal m=3. ... The experiments have revealed banana-like anticyclonic vortices between the spiral arms in corotation region, drifting together with the spiral arms around the vessel axis, so that the joint spiral-vortex structure is formed. ... Nezlin M.,Rulov A., Snezhkin E. N., Trubnikov A. S., , Self-organizaion of spiral-vortex structures in shallow water with repid differenial rotation , Sov.Phys.JETP, 1987, v.65(1), pp.1-4. ...

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• Vortex structure of Milky Way
• Further Data Types
• Results scientific researchs 18

. The UNIX file system is organised as a hierarchy of directories starting from a single directory called root which is represented by a / (slash). Imagine it as being similar to the root system of a plant or as an inverted tree structure. Immediately below the root directory are several system directories that contain information required by the operating system. The file holding the UNIX kernel is also here. UNIX system directories . Home directory . Pathnames .

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• The Structure of HTML 3.0 Documents
• Entering carriage returns
• The Body Element and Related Elements

Университет . ... Наука Патенты Topological types of crystal structures . ... Самарский государственный аэрокосмический университет имени академика С.П. Королева . национальный исследовательский университет)" . ... Тел.: 846) 335-18-26 Факс: (846) 335-18-36 . Содержание Интернет-портала СГАУ: . тел. +7 (846) 267-45-60, . e-mail: webmaster@ssau.ru . ... Тел.: (846) 267-44-99 . e-mail: pr@ssau.ru . ... e-mail: tech@ssau.ru . ... СГАУ 2016 http://ssau.ru | http://сгау.рф | ...

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• Aircraft Structures Residual Strain Research Laboratory (NIL-31)
• Aircraft Structures Science and Research Institute (NII-202)
• Serezhkin Viktor Nikolaevich

... Ciel Espace, le magazine qui vous guide toujours plus loin . ... Ciel Espace, nouvelle formule, c'est . ... des pages consacr†йes †а la publication de vos photos Mais c'est aussi une vraie communaut†й avec laquelle partager votre passion et nourrir votre curiosit†й. Accueil DтАЩ†йtranges structures rocheuses sur Mars . ... Pour en savoir plus sur les explorations men†йes par Opportunity, †йcoutez le podcast Opportunity, †зa roule sur Mars , avec Fran†зois Forget, surle site cieletespaceradio.fr . ...

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• Le trou noir de la Voie lact†йe †а la di†иte | Ciel et Espace

. Head of the project: A.F.Kholtygin

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• Model realization and some results
• Vladimir P. Reshetnikov's Home Page
• Database of Optical Properties -- Level: subsubpage

... Files with sunspot magnetic fields data ============================================== Column Format Description ______________________________________________ 1-2 I2 Day of month 3-4 I2 Month (numerical) 5-8 I4 Year 9 A1 Blank 10-13 I4 UT in hhmm 14 A1 Blank 15-19 A5 Sc - atmospheric flutter in arc sec 20 A1 Blank 21-25 A5 S - quality of the Sun image 26-27 A2 Blank 28-31 A4 Number of sunspots (numbering from unit every day ) 32 A1 ...

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• Datafile structure
• structure

. Composition | Objectives | Capabilities and samples | Request for work | Back to main page . If you have any questions, please contact us: rp@iszf.irk.ru . http://esceir.iszf.irk.ru/lchmen/ris1en.htm . Last modification: 2.06.01.

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• East Siberian Center for the Earth's Ionosphere Research. Modelling, secondary
• East Siberian Center for the Earth's Ionosphere Research. Incoherent scatter