Instrument Summary -- Why Use the GHRS? Here we provide a brief overview of the basic properties of the GHRS. ... The GHRS can obtain spectra from about 1150 to 3200 . ... The repeatability of fluxes is even better, being better than 1%; i.e., it is possible to compare measures of the same wavelength in the same star at different times to within 1% for observations with the LSA. ... The source to be observed may be placed in a Large Science Aperture (LSA) or a Small Science Aperture (SSA). ...

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• Determinations of Dust Scattering Properties
• Metallicity Effects on Dust Properties in Starbursting Galaxies
• Scattering Properties of the Dust in the Reflection Nebula IC 435

... 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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• Arcetri Extragalactic Group
• Client-Side JavaScript Guide

... Bad Astronomy . ... Bitesize Astronomy . ... Last week's Snack talked about how black holes can affect the environment around them in such a way as to be very bright . ... It's a common misconception that black holes always have matter swirling into them. ... As this matter gets closer and closer to the black hole it piles up and a large, fairly flat disk forms. This is called the accretion disk , because matter from this disk accretes (that is, falls in) on the black hole. ... 2008 Phil Plait. ...

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Next: Extinction properties (transmitted radiation) . ... The notes in their current form concern only 2 but main for astronimy aspects of the optical properties of cosmic dust - the ability to extinct and polarize transmitted radiation. The corresponding obervational effects the extinction and polarization (not due to scattering) plaied and plays till now the primary role in astrophysical effects of cosmic dust considered in the literature. ... Extinction properties (transmitted radiation) . ...

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• Astronomy Electronic Preprints and Publications
• Database of Optical Properties -- Level: subpage
• Extinction properties (transmitted radiation)

Stellarium 0.12.3 . ... Classes . ... FileљStructure . ... SatellitesListFilterModel Class Reference . Custom proxy model allowing filtering by satellite group and flag. ... getFilterFlag () const . ... setFilterFlag (const SatFlag &flag) . QStringљ . ... setFilterGroup (const QString &groupId) . ... setSecondaryFilters (const QString &groupId, const SatFlag &flag) . ... Definition at line 27 of file SatellitesListFilterModel.hpp . ... QString SatellitesListFilterModel::filterGroup . ...

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• Stellarium: Ocular Class Reference
• Stellarium: Telescope Class Reference
• Stellarium: MeteorMgr Class Reference

Next: PULSATION PROPERTIES Up: EXTREME HELIUM STARS: PULSATION Previous: EVOLUTION MODELS . ... These include a detailed comparison between models which predict evolution tracks and surface composition for a given stellar mass and accurate observations of stellar compositions and dimensions. ... Stellar pulsations provide much more powerful tools for determining stellar masses. ... Next: PULSATION PROPERTIES Up: EXTREME HELIUM STARS: PULSATION Previous: EVOLUTION MODELS Simon Jeffery . ...

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• Armagh Observatory
• PULSATION PROPERTIES
• Atmospheres

The Local Volume HI Survey (LVHIS) BЁrbel Koribalski a CSIRO Australia Telescope National Facility The `Local Volume' -- the sphere of radius 10 Mpc centered on the Local Group -- includes at least 500 known galaxies. ... To expand and deepen our knowledge of the nearby Universe several teams are currently targeting LV galaxies, among them the "Local Volume HI Survey" (LVHIS; Koribalski et al.), the "Faint Irregular Galaxies GMRT Survey" (FIGGS; Begum et al.) ... Koribalski et al. ...

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• Determining Gains and Polarimetric Properties - GPCAL
• casacore: casa::HDF5HidProperty Class Reference
• Pulsar Group Main/Home Page

The integers $ a_n=\sum_{k=0}^n{\binom nk}^2{\binom{n+k}k}^2, n=0,1,2,... $ appear as denominators of rational approximations to $\zeta(3)=\sum_{k=1}^\infty k^{-3}$ in Apery's proof of the irrationality of $\zeta(3)$. The sequence satisfies a polynomial recursion, namely, $ (n+1)^3a_{n+1}-(2n+1)(17n^2+17n+5)a_n+n^3a_{n-1}=0$, where $n=0,1,2,...$, and admits several curious congruence properties. ... Site design by Paul Zinn-Justin (2005) ...

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• Conference Global Fields
• Conference "Zeta Functions"
• Qualitative properties of reaction-diffusion equations (Spring 2009)

Next: ZGSC (Compressed GSC) and XSKYMAP . ... This is a preliminary report on an investigation of the quality and properties of plates digitized during creation of the Guide Star Catalog (GSC). The results will be vital for reclassifying GSC objects. ... Many objects are measured on more than one plate, and thus have multiple catalog entries. ... Among the shortcomings of the GSC are: biased magnitudes and incorrect classifications for certain objects, presence of artifact objects. ...

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• The Astrometric Properties of the NOAO Mosaic Imager
• ADASS 2003 Conference Proceedings
• Stochastic Relaxation as a Tool for Bayesian Modeling of Astronomical Images

Molecular clouds in the central 200 pc of the Galaxy (the Central Molecular Zone ) exhibit different (and more extreme) physical properties than those in the disk, yet because this is the closest galactic nucleus, detailed studies of this region can provide insight on galactic nuclei in general in the nearby universe. ... In this talk I will present a case study of one of the clouds - a dense and unusual cloud, GCM0.253+0.016 - also known as The Brick . ...

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• Dougal Mackey - Research
• Raquel Salmeron - Research Interests and Experience

. Mars is "behind" the sun from the earth's point of view and is therefore not visible in the nighttime sky (i.e. its up in the daytime). Venus it at greatest elongation and appears in the western sky as a bright object for 2-3 hours after sunset .

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• Orbital Properties of the Earth

. Main Page . Related Pages . Classes . Files . Class List . Class Hierarchy . Class Members . Properties of carbonaceous grains. More... #include < dustmodel.h > . List of all members. double . qgra . double . axi . Properties of carbonaceous grains. The documentation for this struct was generated from the following file: . dustmodel.h . Generated on Fri Jul 11 07:32:08 2008 for DUST by 1.5.5

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• PPT Slide
• DUST: dust_nmoded Struct Reference
• DUST: silprops.h File Reference

... 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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The possibility to have Visitor Instruments at the VLTI has been granted to permit innovative observations by teams using stand-alone instruments, free from a substantial fraction of the requirements for fully automated VLTI general use instruments. In addition, the Visitor Instruments could provide a powerful scientific/technical test bench for new instrumental concepts, eventually to be incorporated later in VLTI facility instruments. ... a thorough technical description of the instrument, . ...

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• Introduction
• Sample Properties
• Help for Night Report / Progress Pages

Планета Земля и Луна . ... Космическая защита . Луна . Фотографии . ... Строение Луны . ... Страница: Начало одиссеи , Экспедиции , Море Кризисов , "Аполлон-8" , "Аполлон-9" , "Аполлон-10" , "Аполлон - 11" , E-8 "Луноход" , Испытания Л-1 , Луноход - 1,2 , КА "Луна 1-24" , КА "Луна-9" , Луна от КА СССР ; . Луна - наш космический спутник . ... Снимки Луны от аппаратов серии Луна и Зонд (СССР) . Фотографии космических аппаратов серии "Луна" (также Луноходы) и "Зонд" - СССР . ... Зонд 3 . ...

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. Next: A Quick Look Up: Spectral-Line Observing at AO Previous: THE SOURCE LIST . This section describes using the AO-Control GUI - a graphical user interface (GUI) to the Arecibo observing/datataking system - for spectral line observations. If you would like more information on the general properties of the GUI, go to http://www.naic.edu/ aoui . Subsections . A Quick Look . The Details . Useful Stuff . koneil@naic.edu

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• Available Receivers
• THE SOURCE LIST
• Heiles Symposium Presentations

... Observations of the Moon eclipse on 17.09.97 have shown the Moon details contrasts had decreased and the total radio brightness had fallen at all observed frequency range (from 10% at 1.38 sm down to 2.5% at 13 sm). The fall of the Moon radio brightness has been detected during the eclipse at decemeter waves for the first time. ... Radio emission of the Copernicus crater at 1.38 and 2.7 sm has been detected for the first time. ...

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• Structure and properties of IRC+10216
• Spectral energy distribution

... Physical Properties of Crystals . ... The course is an introduction into crystal physics and consists of two introductory parts devoted to the basics of crystallography and tensor analysis and six main chapters in which the physical phenomena in anisotropic medium are described by the example of the elastic, electrical and magnetic crystal properties. The effect of symmetry is also discussed. ... Effect of symmetry on crystal properties. ... Effect of symmetry on crystal optical properties. ...

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• Laboratory for Spectroscopy of Molecular Structures
• CONTENTS
• LHPP ISSP RAS

... The most important consequence of orbital eccentricity for the evolution of rotators can be understood without detailed calculations, and suggests the existence of two different types of binary systems separated by a critical eccentricity, (Gnusareva and Lipunov, 1985)[ 56 ]). ... Therefore, for a small part of its life the rotator will be in a mixed EP-state, being in the propeller state at periastron and at the ejector state close to apastron. ...

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• Introduction
• Physicists on the Money
• The Gravimagnetic Parameter

... 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
• Group IAG
• The ROSAT AGN