HUBBLE SPACE TELESCOPE DAILY REPORT #1596 PERIOD COVERED: 0000Z (UTC) 03/21/96 - 0000Z (UTC) 03/22/96 Daily Status Report as of 082/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed WF/PC-2 5939 (Evolution in the Isotropic Properties of = BL Lac Objects) The WF/PC-2 was used to make observations of the BL Lac object = PKS1538+14 in order to study its evolution and isotropic properties. ... The observations were = completed as planned, and no anomalies were reported. ...

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• http://www.stsci.edu/ftp/observing/status_reports/old_reports_01/hst_status_05_23_01
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_03_19_97
• http://www.stsci.edu/ftp/observing/status_reports/old_reports_99/hst_status_03_31_99

... Stellar Evolution . Nucleosynthesis in Stars . The Evolution of Star Clusters . JAVA Physics Lab . Alternative Energies Class . Steve Kevan's Physics 251 Class . ... Talk on Solid State Physics of CCD detectors . Talk on Cosmological Issues . ... Digital Spectra of Stars . NETexperts E-mail List . The Electronic Universe Project e-mail: nuts@moo.uoregon.edu ...

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• Astronomy HyperText Book: Stellar Evolution

Next: EVOLUTION MODELS Up: EXTREME HELIUM STARS: PULSATION Previous: EXTREME HELIUM STARS . The characteristic surface properties, effective temperature , surface gravity and composition , of EHes have been summarized by Jeffery (1996). ... Helium: ( ) By definition, helium dominates the atmospheric abundances. ... This is supported by a correlation between N and Fe abundances in EHes. ... Next: EVOLUTION MODELS Up: EXTREME HELIUM STARS: PULSATION Previous: EXTREME HELIUM STARS Simon Jeffery . ...

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• Stars Beyond Maturity
• EXTREME HELIUM STARS
• V652HER AND MERGED BINARY WHITE DWARF MODELS

... at the ISSP RAS. ... MSU student Kostretsova N.B. successfully defended her thesis entitled "Investigation of Thermal and Chemial Expansivity of Ceria-Based Solid Solutions". ... V.A. Kolotygin successfully defended his PhD thesis "Perovskite-Like Oxide and Composite Anode Materials for Solid Oxide Fuel Cells: Functional Properties and Electrochemical Behavior in Contact with Gallate- and Silicate-Based Solid Electrolytes" and was awarded PhD degree in the area of Materials Science and Engineering ....

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• Physical Properties of Crystals
• LPCBC: Abstract 2_26

... Pre-university education . ... Samara region . ... University at a glance . ... A group of young scientists of Samara University under the guidance of the candidate of chemical sciences Yevgeniy Aleksandrov began to make the most extensive database in the world for the structure and physical properties of crystalline coordination polymers. ... The idea of making a database for coordination polymers already exists in the scientific community of the world. ... SAMARA STATE AEROSPACE UNIVERSITY . ...

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Next: Supernova Explosions Up: No Title Previous: X-ray Luminosity Evolution . The origin of cosmic rays (CR) (especially of very high energies, >  eV) until now has been one of the unsolved problems in modern astrophysics. It is unclear as yet whether one universal mechanism of relativistic particle formation in our Galaxy operates or not, and if there are several different mechanisms, what is their relative contribution to CR formation. ... compact X-ray stars in binary systems. ...

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• Mixing types of E-P-A binary systems with non-zero orbital eccentricity
• Evolution of the Double Neutron Star Merging Rate andthe Cosmological Origin of
• Introduction

... We suggest simple method of the selection of distant galaxies based on their radio properties. ... RC0015+0503a , RC0015+0503b , RC0015+0501 , RC0034+0513 , RC0038+0449 , RC0042+0504 . ... RC0105+0501 , RC0110+0500 , RC0117+0503 , RC0126+0502 , RC0133+0459 , RC0135+0450 , RC0137+0539 , RC0143+0505 , RC0152+0453 , RC0154+0459 , RC0159+0448 . ... RC0209+0501b , RC0213+0516 , RC0226+0512 , RC0250+0512 . ... RC0302+0456 , RC0308+0454 , RC0311+0507 , RC0318+0456 , RC0355+0449 . ...

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... This chapter documents all the JavaScript objects, along with their methods and properties. ... Full entries for each object appear in alphabetical order; properties and functions not associated with any object appear in Chapter 2, "Top-Level Properties and Functions." ... Tables included in the description of each object summarize the object's methods and properties. Full entries for an object's methods and properties appear in alphabetical order after the object's entry. ...

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• Slide 7
• Local Universe
• Virgo Group - Gravitational Wave basics

... Home . ... Main . ... The pulsar group is part of the Australia Telescope National Facility , a division of the CSIRO . The ATNF operates the Parkes radio telescope where the majority of our observations are carried out. ... The ATNF Pulsar Educational Page gives a broad overview of pulsar properties, observations and current research projects. ... Our group developed the web-based ATNF Pulsar Catalogue , which provides comprehensive information on all published pulsars. ... Pulsar Catalogue . ...

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• PPTA Dashboard | Projects
• Basic Properties
• The completeness and reliability of threshold and false-discovery-rate source

Next: Redshift Distribution Up: Sample Identification Previous: Previously Identified Sources . ... In Figure 3, we plot the redshift distribution of DXRBS FSRQs opposite that of the 1 Jy and S4 samples. In Figure 4, we plot the redshift distribution of DXRBS BL Lacs opposite the Slew and 1 Jy samples. ... The apparent deficit of objects at the very highest luminosities is a result of the smaller area of sky covered by DXRBS compared to, e.g., the Slew and 1 Jy samples. ...

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• ESO - Thesis Topic: The dawn of planets: structure and evolution of
• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
• Marina Rejkuba's Web Site

... Galaxy Evolution home . Cavendish Astrophysics . ... Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . ... Radio sources are among the most powerful of the family of Active Galactic Nuclei (AGN). ... The overall properties of radio sources are well predicted by analytical models of self-modifying evolution of the radio source which we have developed, and many of the more unusual structures observed can be reproduced using computational models. ...

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• Galaxy Evolution Bojan Nikolic web pages (r. 329)
• Galaxy Evolution: Regulation of the ISM and Star Formation
• Astrophysics Group Galaxy Formation and Evolution

Next: Examples of data contained Up: Electronic database Previous: Future plans . In astrophysics, the optical constants mainly are used to calculate the optical properties of scatterers, i.e. cross-sections, scattering matrix, etc. ... Optical properties derived from such models have been discussed in some books (see, e.g., [ 2 , 3 ]) and in principle can be calculated by using various light-scattering tools which are freely available via the internet [ 4 ]. ...

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• Vladimir P. Reshetnikov's Home Page
• Database of Optical Properties -- Level: subpage
• Extinction properties (transmitted radiation)

A1625 2002-Feb-01 15:13:28 Technical Page Proposal Type: Long-term General Category: Astronomy Sub-Category: Spectroscopy Observation Category: Extragalactic Total Time Requested: 45 Hours Proposal Title: Properties of the ISM of a sample of the most isolated galaxies: Atomic gas content. ... Our source is the Catalog of Isolated Galaxies and our sample contains 760 galaxies for which we are building a multiwavelength database. ... This proposal requires coordination with GPS L3 at 1381 MHz. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/GrogintagA1584tp.ps
• http://www.naic.edu/vscience/schedule/2015Spring/KannappantagA2812.pdf
• http://www.naic.edu/vscience/schedule/2014Fall/FerdmantagP2789.pdf

... The sky distribution of the BCGs from the HSS sample is shown in Fig. 6 together with BCGs from the SBS and Case surveys (Izotov et al. [ 1993b ]; Pustilnik et al. ... First, we compare the apparent magnitude distributions of the three samples. ... The similar behaviour of the faint end of the apparent magnitude distributions infers that the Northern BCG sample may have a similar completeness down to this limiting magnitude. ...

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• The very metal-poor local dwarf galaxies
• Properties
• AstroGrid Registry FAQ

A completely new possibility of Fortran 90 is recursion. Note that it requires that you give a new property RESULT for the output variable in the function declaration. ... Here follows two examples, first recursive calculation of the factorial, then recursive calculations of the Fibonacci-numbers. ... The listings of the routines follow, the output variables are called FAC_RESULT and FIBO_RESULT , respectively. ... Not only functions but also subroutines can be recursive. ...

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• Media types
• ApSA courses
• Visual effects

... This implies powerful stability and collimation taking into account that different instabilities can affect the evolution of jets. ... Thus, jet stability has been a significant research subject during the last decades. In this talk, I will present some recent results on the linear and non-linear stability analysis of non-relativistic magnetized jets carrying helical magnetic fields. ... I will discuss the non-linear evolution of jets with the aid of three-dimensional numerical simulations. ...

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• http://www.mso.anu.edu.au/seminars/abstracts/20151119-1100.html
• http://www.mso.anu.edu.au/seminars/abstracts/20141120-1100.html
• http://www.mso.anu.edu.au/seminars/abstracts/20150213-1400.html

... 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 . ...

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• Spectral energy distribution
• About laboratory
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and

... The Science Operation Department is composed of Astronomers, Telescope Instruments Operators(TIOs) and Data Handling Administrators(DHAs). ... Astronomers have proposed several methods to quantitatively measure the amount of turbulence above the telescope, which the most common ones is Differential Image Motion Monitor (DIMM). In optical testing, the Hartmann test is the common method to test the quality of optical components. ... Hartmann mask consists of 48 lenses. ...

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• General information

... Emission Line Properties of AGN from a post-COSTAR FOS HST Spectral Atlas" . ... Emission line measurements: - FORMAT , and DATA . ... Evidence for a Strong NV/CIV Correlation Between Emission and Absorption Lines in AGN" . ... Emission Line Properties of AGN from a pre-COSTAR FOS HST Spectral Atlas" . ... The Hubble/ROSAT Continuum and Ultraviolet Line Emission Study (H/RCULES) of AGN enables characterization of: . Spectral energy distributions from X-ray to Radio. ... Emission line properties. ...

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• Conclusions
• Pat Slane: Research
• Fits to Evolutionary Models

... January 16, 1998 . Dusting Spiral Galaxies . Credit: W. Keel and R. White ( U. Alabama ), NASA . Explanation: How much dust is in spiral galaxies? ... This striking, detailed Hubble Space Telescope image of dust in the outer reaches of a foreground spiral galaxy (left) back lit by an elliptical galaxy offers an elegant approach to providing the answers . As expected, dust lanes in the foreground galaxy seem to be associated with spiral arms. ... About APOD > . ... NASA Technical Rep.: ...

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• Zen: CASDB
• Intro
• APOD: 2014 September 26 - MAVEN at Mars