... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

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• Initial parameters of compact stars
• Initial Distributions of Binary Parameters
• The Gravimagnetic Parameter

Galushina T., Bykova L., Letner O., Baturin A. Tomsk State University Russia 1 Investigation Dynamics Asteroid of of 2 Solving problems construction of numerical model of asteroid motion with account chosen perturbed factors; asteroid orbit improvement according to positional observations; construction of initial probabilistic domain by linear and nonlinear methods; study of evolution of initial probabilistic domain; revealing of ...

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• http://www.gao.spb.ru/english/as/j2014/presentations/suvorkin.pdf
• Pulkovo NEO Page: Ephemeris Support

... ratios Evolution Equations with · Now write · Evolution equations now · Define trajectories via Cosmic Trajectories Dust =0 de Sitter phase Radiation =1/3 Initial singularity Cosmic Trajectories · For a range of initial conditions, models re-focus around the flat ... case · For decoupled matter and radiation can solve the equations exactly · Solutions governed by two constants: Non-Euclidean Geometry · Axioms of ...

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• http://www.mrao.cam.ac.uk/galevol/jsabater-Cambridge.pdf
• Paper I: Method Bojan Nikolic web pages (r. 329)
• De-convolution of a Gaussian beam from planetary observations Bojan Nikolic web

... 0 ) = Z '' '' 0 [(1 \Gamma '')'' 1=2 sin 2 i sin 2!] ... We use the similarity theory to present the non--dimensional period T \ Lambda of the evolution of the parameters '' and i as a product of the independent factors: T \ Lambda = \ Gamma (4=15)(a \ Gamma3 =2 \ Lambda =LD )jL c (c 1 ; c 2 )j. Here LD = Ї k \ Lambda a \ Gamma3 k \ Lambda '' \ Gamma3 =2 k Ї \Gamma1=2 \ Lambda is the non-- dimensional parameter of disturbances similarity dependent on the dynamical characteristics of the ...

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• http://www.ipa.nw.ru/conference/2002/sovet/PS/BYKOVA1.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/BORDOVIT.PS
• http://www.ipa.nw.ru/conference/2002/sovet/PS/PITJEVA.PS

... Column 1 gives the object name from the Case or Markarian catalogs. ... For Markarian galaxies the errors of coordinates usually lie inside 2'' (Lipovetsky [ 1983 ]). Column 4 gives the eye-estimated apparent blue magnitudes according to the same sources. ... Other names of a galaxy we give in column 7. ... In column 3 we cite the original emission-line code of the galaxy for the strength of [O III ] doublet according to the Case catalog (s - strong, m - medium, w - weak). ...

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• Parameter estimation
• Reducing the observations
• HyperLEDA documentation: parameter: vmaxg

Welcome to the Starburst and Galaxy Evolution website.

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• Fundamental Parameters, Integrated Red Giant Branch Mass Loss, and Dust
• ST ScI Preprint #1359a
• Precision Photometry at the LMC Center: Simulating Post-COSTAR HST Observations

... Second, the observatory can control the configuration, test data analysis procedures, and provide calibration solutions with the help of instrument models. This paper presents the VLT object-oriented framework for the development of ETCs (Exposure Time Calculators) and data simulators. ... Instrument simulations are being developed for the purpose of predictive calibration, instrument configuration control, and evaluation of data analysis procedures. ...

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• Modern CCD Observations of Moving Celestial Objects: Algorithms and Software
• Enhanced HST Pointing and Calibration Accuracy: Generating HST Jitter Files at
• ADASS 2003 Conference Proceedings

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• The Case for Non-Zero Lambda

... A model for the chemical evolution of a disk galaxy is presented. The model reproduces all the basic . ... investigations of the star formation history. ... the galaxyЫand incorporating a delay in the onset of star formation make it possible to model different scenar- . ios for the evolution of a galaxy's luminosity. ... evolution of massive galaxies. ... of reconstructing the star-formation history and galactic luminosity from observations of galaxies at different . ...

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• Future of the Galaxy

Modelling Protostellar Disks Sarah Maddison Centre for Astrophysics and Supercomputing Swinburne University Overview · Types of circumstellar disks : ­ protostellar disks ­ circumbinary disks ­ protoplanetary disks · Modelling disk - important parameters: ­ Mdisk, Rdisk, H(r), i, T(r,z), (r,z)... ­ grain properties Introduction to PS Disks · Disks are a natural by- product of star formation process · Indirect evidence for ... Fuor and Xor outburst) convection in accretion disks? ...

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• Making a Fake Observation
• Late Stages of Stellar Evolution
• casacore: Fitting_module

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Investigations of the ionospheric response to strong magnetics storms which are usual for our latitudes, are of great interest. ... In the figure, we present ionospheric parameter dynamics during three perturbed days in July 2000. ...

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• East Siberian Center for the Earth's Ionosphere Research. Capabilities and

Next: Program use Up: Description of program searchdup Previous: Description of program searchdup . Parameter input is done with a graphic user interface. ... Input file: Name of the input catalog file. It has to be formatted, one record per source/observation, according to the format used in the Arcetri observations and source archives. ... Minimum number of observations per source Source with less than this number of independent observations are not included in the output file . ...

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• Arcetri Star-formation Group Research Topics
• research field
• Determination of the Detector Parameters

XMM-Newton Science Analysis System . ... yes . ... pn source region expression for spectral analysis . ... pn background region expression for spectral analysis . ... mos1 source region expression for spectral analysis . ... mos1 background region expression for spectral analysis . ... mos2 source region expression for spectral analysis . ... pn source region expression for timing analysis . ... mos1 source region expression for timing analysis . ... mos2 source region expression for timing analysis . ...

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... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...

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• ESO - Studying the Cosmological Evolution of Galaxy Clusters with (Sub-)mm
• Parameters
• Quality Control: Image flats

... The search for distant objects which can be both galaxies and quasars is one of the most important problems of observational astrphysics, because it allows one to determine cosmological parameters connected with the time of appearence and evolution of stellar systems, large scale structure of the Universe. ... Radio galaxies are important objects to be studied because they are sources of infrared-optical-ultraviolet continuum, emission lines and continual radio emission. ...

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• Optimization of spectroscopic observations
• проект SCORPIO-2: parameters
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Physics and

... the radiative transfer equation (RTE) for the randomly-irregular magnetized plasma has been derived on the base of general grounds of the multiple scattering theory . ... Solutions of several absolute tasks of the scattering theory have been obtained (on the optical depth of the ionospheric plasma layer, on the value of radio wave anomalous attenuation, on anomalous refraction, on the backscattered signal intensity for the source being placed within a plasma layer). ...

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• Vladimir Marsakov Publication List
• Vladimir Marsakov Abstracts

PHYSICAL PARAMETERS FOR SUBDWARF B STARS WITH COMPOSITE SPECTRA R. AZNAR CUADRADO, C.S. JEFFERY Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland For many years, the evolutionary origins of subdwarf B stars remained a mystery. ... The infrared triplet of ionized calcium was recognised as a good in- dicator of a late-type companion in composite sdB spectra [5] and is an excellent measure of cool star surface gravity. ... Aznar Cuadrado, R., and Je ery, C.S. (2001) A&A 368, 994. ...

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• White Dwarf Merger Movie
• Refereed Journal Publications 2004
• The Chemical Evolution of FGSge

lsst.coordConv љ unknown . ... Classes . ... coordConv::OtherCoordSys Class Reference . ... OtherCoordSys (std::string const &name, double date=0, DateTypeEnum dateType= DateType_None , bool isMean =false) . ... virtual Coord љ . ... CoordSys (std::string const &name, double date, DateTypeEnum dateType, bool isMean , bool canConvert ) . ... convertFrom ( CoordSys const &fromCoordSys, Coord const &fromCoord, Site const &site, double tai=0) const . ... virtual Coord coordConv::OtherCoordSys::removePM . ...

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• lsst.coordConv: coordConv::FK4CoordSys Class Reference
• lsst.coordConv: coordConv::FK5CoordSys Class Reference
• lsst.coordConv: coordConv::ICRSCoordSys Class Reference

... An error involving a missing tasks parameter indicates that the parameter file may have changed between the last time the task was used and the current version. ... If still in trouble, delete the parameter file in `myiraf/uparm' corresponding to the task (the names are somewhat contrived, but with a bit of imagination it is not too difficult to identify the right one). ... The imcnts task and region masks . ... A region descriptor of the kind: . CIRCLE(403, 403, 22.5) . ... See `help regions'.) ...

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• The AstroStat Slog parameter estimation
• The AstroStat Slog Blog Archive A test for global maximum
• The AstroStat Slog Blog Archive Likelihood Ratio Test Statistic [Equation of

... Proposal Type: General Category: Sub-Category: Observation Category: Total Time Requested: Minimum Useful Time: Prop osal Title: Regular Astronomy Spectroscopy Galactic 26 Hours 2hr The evolution of massive Hi-GAL clumps towards high-mass stars: constraints on physical parameters from the H2CO 6-cm transition ABSTRACT: The Hi-GAL survey gives us a unique opportunity to study the process by which molecular clouds condense into clumps and cores, and then into massive stars. ...

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• http://www.naic.edu/~astro/chicago2/talks/Furlanetto-Cosmology_and_Future_Radio_Telescopes.pdf
• AGES Database Search
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution