Stellarium 0.12.3 . ... Classes . ... Protected Attributes . StelVertexBufferBackend Class Reference abstract . Base class of all vertex buffer backends. ... StelVertexBufferBackend (const QVector< StelVertexAttribute > & attributes ) . Construct a StelVertexBufferBackend , specifying attributes of the vertex type. ... virtualљ . ... virtual voidљ . ... Data members of the vertex must match vertex attributes of the buffer. ... const Attributes StelVertexBufferBackend::attributes . ...

... Translate Abstract . ... Structure and properties of IRC+10216 . ... AA(Stockholm Observatory, SE--133 36 Saltsj baden, Sweden), AB(Special Astrophysical Observatory, Nizhnij Arkhyz, Karachaevo-Cherkesia, 357147, Russia), AC(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany), AD(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany), AE(Max-Planck-Insitut f r Radioastronomie, Auf dem H gel 69, D--53121 Bonn, Germany) . ... Abstract Text . ...

... Abstract Return summary information for a specified segment in a specified EK. ... Detailed_Output segsum is a pointer to an EK segment summary. ... Loop through the segments, dumping the desired summary information for each one./ printf ( \n \n Segment summary for file %s\n \n \n , ek ); for ( segno = 0; segno nseg; segno ++ ) { ekssum_c ( handle , segno , segsum ); printf ( ======================================== ======================================== \n ...

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 . ...

... Next: An Abstract Data Up: Data Models and Previous: What is an . ... We describe a possible data structure designed to improve propagation of physics information in an analysis system, and an associated subroutine library for combining physical units. ... It has the size and shape of the physical data array, and its pixel values represent the exposure time for that element of the array. ... A Unit handling library parses physical unit definitions, and provides simple routines to combine them. ...

... 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 . ...

... Meta Index . Several conventions are described for passing around data in the SAS, such as parameter names, file structure, attribute names, column names etc. ... Event lists . Event status . Errors . Note . ... Parameter names . ... Attributes . OGIP compliance . Relevant OGIP standards . XMM-specific extensions of the OGIP standard . Automatically generated attributes . ... Column names . Events lists . ... Index . ...

... The theory of the large scale structure of the universe . ... The theory of perturbation growth is considered with attention to acoustic oscillations of the radiation-dominated plasma and their attenuation before and during recombination, the growth of small perturbations in the neutral gas, the nonlinear growth of perturbations leading to the formation of compressed gas layers - pancakes, and the further fate of pancakes leading to their decay into galaxies and protoclusters of galaxies. ...

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: The dawn of planets: structure and evolution of protoplanetary disks with ALMA . ... ALMA . ... Observing with ESO Telescopes . ... At ESO we have primary responsibility for the determination of the stellar and star-disk interaction properties using VLT/XShooter spectroscopy and for the study of the dust properties in protoplanetary disks from observations at submm and radio wavelengths with ALMA and the VLA. ...

... Here we describe and discuss the various data entities (structures) that MIDAS recognizes. ... The paragraphs below describe the structure of descriptors, and keywords, and the methods for specifying the individual data values in images and tables. Note is no special syntax for file names in MIDAS. ... If you do want to use a file name with these special characters in a COMPUTE/IMAGE command you have to enclose the full name in quotes, i.e. Midas 456> COMPUTE/IMAGE res = 12 + "quasar01 + 12.bdf" . ...

... Programme . ... Presenter: Steven Tingay (International Centre for Radio Astronomy Research) . Abstract: I will review the history of high angular resolution observations of Centaurus A, concentrating on the structure and evolution of the sub-parsec-scale radio source, its nuclear environment, and recent results revealing parsec-scale structure in the kiloparsec-scale jet. go back . CSIRO 2009 Legal Notice / Privacy Statement Last modified: 15/11/2010 ...

... 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. ...

... AAS link ] . ... Our internal perspective makes it difficult to determine the spiral structure of our own galaxy. ... H I absorption, on the other hand, traces colder, denser gas that should be more confined in discrete clouds and perhaps discrete spiral arms. In addition, H I self-absorption (HISA) requires background H I emission at the same velocity as the foreground absorbing gas, thus introducing a much-needed constraint on the large-scale sightline geometry and kinematics. ...

We investigate models for main-sequence and horizontal-branch (HB) stars constructed using the Carson opacities and make comparisons with models based on the Cox-Stewart opacities. ... The drop in the hydrogen-shell luminosity due to the helium-core expansion during HB evolution is greater than that obtained with the Cox-Stewart opacities. ... Studies of main-sequence (MS) stars lead to agreement with Stothers' (1974a,b, 1976) results for homogeneous models constructed with Carson opacities. ...

... Most HTML elements are identified in a document as a start tag, which gives the element name and attributes, followed by the content, followed by the end tag. ... To identify the document as being HTML 3.0, it is recommended that documents start with the prologue: <!doctype HTML public "-//W3O//DTD W3 HTML 3.0//EN"> . ... HTML 3.0 documents formally have the following structure: <HTML> <HEAD> head elements .. ... HTML> . ... The permitted syntax of HTML 3.0 compliant documents is specified by the...

... 1) The MS lower envelopes for groups of stars with different metallicities turn out to be coincident. ... 4) The conformation of the kinematics of stars within narrow ranges ob b-y with the ages derived from isohrones reveals that, at Z < Z , the isohrone ages seem to be increasingly overestimated with growing b-y . ... At a given metallicity, they have a much narrower MS and the locus of their MS lower envelope seems to be brighter for the metal-rich group of stars. ...

... 2) Physics Department, University of Puerto Rico at Rio Piedras, P.O. Box 23343, San Juan, Puerto Rico 00931 . ... We report the density structure of the ultracompact HII regions G35.20-1.74, G9.62+0.19-E, and G75.78+0.34-H2O. The density profiles are derived from radio continuum emission at wavelengths from 6 to 0.3cm. In the case of G35.20-1.74, a cometary UC HII region with a core and a tail, the spectrum of the core varies as Snu~nu^(0.6), implying that the density structure is ne~r^(-2). ...

... Klien topological field theory and Hurwitz numbers of complex and real algebraic curves . Gzipped postscript ] . ... Text ] . ... Astroidal geometry and hyperbolic polynomials . ... Symmetric powers as algebraic variety . ... Abelian Lagrangian Algebraic Geometry and ALAG-quantization . ... Symplectic singularities in algebraic geometry . ... Algebro Geometric methods in symplectic geometry . ... Classification of the real simple Lie superalgebras of vector fields . ...

... Structure of superconducting single crystals of (2201) thallium cuprate (Tl 1.85 Cu 0.15 )Ba 2 CuO 6 , T c =110 K. Abstract: . Single crystals of 2201 phase with various superconducting transition temperatures ranging from nonsuperconducting to 110 K have been obtained. ... A correlation between the structure and properties of Tl-2201 cuprate crystals has been established on the basis of our data and the data reported in the literature ...

... Department of Physics & Astronomy, Rutgers University, PO Box 849, Piscataway, NJ 08855-0849, U.S.A. Rich cluster CL 0016+16 lies in a large-scale dynamical structure at redshift , and has a strong Sunyaev-Zel'dovich effect. When the X-ray and radio data for CL 0016+16 are interpreted in terms of the cluster distance, this cluster provides the highest redshift datum on the Hubble diagram based on the Sunyaev-Zel'dovich effect, with a Hubble constant of . ... 4 The Hubble diagram . ...