Next: Star Formation Rate and Up: No Title Previous: Calculation of Evolutionary Tracks . To start calculations, we choose the distributions of the initial binary parameters: the mass of the primary ZAMS component, , binary mass ratio, , orbital separation a . ... whereas the mass ratio distribution is not. ... The zero assumption often made is that the mass ratio distribution has a flat shape, that is binaries with a high mass ratio occur as frequently as those with equal masses. ...

Еще в разделе: (Показать все результаты (>478) - xray.sai.msu.ru/ )

• Old neutron star distribution in the Galaxy
• Figures and figure captions
• Initial binary parameters

... Bojan Nikolic web pages (r. 329) . ... We present a Bayesian approach to calculating the coefficients that convert the outputs of ALMA 183 GHz water-vapour radiometers into estimates of path fluctuations that can be used to correct the observed interferometric visibilities. ... Inference of Coefficients for Use in Phase Correction . ... Simulating Atmospheric Phase Errors, Phase Correction and the Impact on ALMA Science . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

Еще в разделе: (Показать все результаты (>1226) - www.mrao.cam.ac.uk/ )

• Inference of Coefficients for Use in Phase Correction
• OOF Reduction Software Bojan Nikolic web pages (r. 329)

... Polar Cap Potential . ... The solar wind propagation delay time calculation used here is conceptually similar to the T(IMF) calculation in Kelly, et al. ... The older continuous data are from key parameter data files. ... Note: Very high values of Solar Wind Speed, Solar Wind Pressure, IMF Magnitude and Bz, and Polar Cap Potential are likely indications that WIND has reentered the Earth's magnetosphere; such data is not indicative of solar wind conditions or impending severe geomagnetic disruption. ...

Еще в разделе: (Показать все результаты (>850) - www.iki.rssi.ru/ )

• Space Weather Dials Interpretation Guide

... Minute Values of Geomagnetic Field Components . ... AA 1868 - Present (3 hourly and daily) (monthly) (yearly) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) KP_AP 1932 - Present (3 hourly and daily) (Lists and histograms of geomagnetic disturbance and Solar Sunspots) AE_HV 1957-75, 78-88 (hourly) AE_MIN 1978-881-6;198903;1990-94 (minute) DST 1957 - Present (hourly) PC 1975 - Present (15-minute) AMANAS 1959 - Present (3 hourly and daily) KMKNKS 1983 - Present (3 hourly) . ...

Еще в разделе: (Показать все результаты (>3533) - www.wdcb.ru/ )

... We present a computer program for modelling energy flux distribution and light curves of eclipsing binaries from far ultraviolet to infrared regions. The Roche model is assumed. Proximity effects of components (reflection of radiation and surface gravity darkening) are taken into account. ... Figure 1: The surface temperature distribution for Algol A-B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation effect. ...

Еще в разделе: (Показать все результаты (>1637) - www.adass.org/ )

• Starlink's Software Distribution System
• Calculating the Position and Velocity Components of HST
• Identification and Analysis of Binary Star Systems using Probability Theory

XMM-Newton CCF Release Note XMM-CCF-REL-183 EPIC-pn spectral response R. D. Saxton 11 November 2004 1 CCF components Name of CCF VALDATE Blocks changed XSCS ag EPN QUANTUMEF 0015.CCF 2000-01-01 FRACTION CHANNEL, FRACTION ENERGY QE TOTAL, EBINS FRACTION NO EPN REDIST 0009.CCF 2000-01-01 NOISE PARAMS, PARTEVENT PARAMS THRESH LOSS NO 2 Changes Recent calibration work has shown that the Epic-pn redistribution function is in practice narrower than that represented in the current matrices. ...

Еще в разделе: (Показать все результаты (>6402) - xmm.vilspa.esa.es/ )

• Procedure
• External SAS packages
• Functionality

... Archives . ... ArXiv] SVM and galaxy morphological classification, Sept. 10, 2007 . ... On the Metallicity-Color Relations and Bimodal Color Distributions in Extragalactic Globular Cluster Systems by M. Cantiello and J. P. Blakeslee . Many observations on globular cluster systems (GCS) show bimodal distributions in color and metallicity space. ... Based on their simulation study, (V-H) and (V-K) are confirmed to be good colors for revealing unbiased bimodal metallicity distributions in GCS. ...

Еще в разделе: (Показать все результаты (>2019) - hea-www.harvard.edu/ )

• Comments on: tests of fit for the Poisson distribution By: hlee
• The AstroStat Slog regularity condition
• The AstroStat Slog Blog Archive [ArXiv] Identifiability and mixtures of

... In this first example, we allow an object to fall onto a small radar unit . The resulting Time-Frequency distribution is shown as a contour plot in Fig. 8 (a). Figure: FIGURE GOES SOMEWHERE IN THIS GENERAL VICINITY . ... Its density plot appears as an image in Fig. ... The response has a very high peak, as evidenced from Fig. ...

Еще в разделе: (Показать все результаты (>2902) - crydee.sai.msu.ru/ )

• Relationship Between Auto Chirplet FF Plane and Radon Transform

... In brief: the frequency-dependent radiative transfer equation is solved for a dust under assumption of spherically-symmetric geometry for its distribution taking into account particle size distribution and quantum heating effects for the very small dust particles. ... Table: Model parameters for IRAS04296+3429. ... parameter . ... hot dust shell) . ... The best fit to the spectral energy distribution of IRAS04296 is shown by heavy solid line (see Table2 for details concerning parameters of the model...

Еще в разделе: (Показать все результаты (>730) - jet.sao.ru/ )

• Determination of atmospheric parameters and calculation of chemical composition
• Iron abundance in the atmospheres of components of the binary system 41...
• harak_e

... Namespaces . Classes . Files . ... File List . ... components . ComponentModels . ... include < casa/aips.h > . include < casa/BasicSL/Complex.h > . include < components/ComponentModels/ComponentType.h > . include < components/ComponentModels/TwoSidedShape.h > . Go to the source code of this file. class . ... All Classes Namespaces Files Functions Variables Typedefs Enumerations Enumerator Friends Defines . Generated on Fri Sep 3 2010 13:07:39 for casacore by 1.7.1 ...

Еще в разделе: (Показать все результаты (>7565) - www.atnf.csiro.au/ )

• casacore: components/ComponentModels/GaussianShape.h File Reference
• The spectral energy distribution of PKS 2004-447: a compact steep-spectrum
• Red synchrotron jets in Parkes quasars

Next: Examples and Photometric Up: Image Restorations of High Previous: Introduction . ... where is the intensity of the point sources (mainly zero apart from -functions at the positions of designated sources) and is the intensity of the background. ... When is zero the objective function becomes the same as that of the standard Lucy-Richardson technique. takes the form of an entropy expression which may be calculated in two ways, relative to a flat background: . ...

Еще в разделе: (Показать все результаты (>13525) - www.stsci.edu/ )

• STScI Preprint #1330
• Software Conditions
• Dust Attenuation in Late-Type Galaxies. I. Effects on Bulge and Disk Components

... Proximity e#ects of com­ ponents (reflection of radiation and surface gravity darkening) are taken into account. ... As an example, we consider the Algol (# Persei) system, where an eclipsing pair (Algol A­B) is accompanied by the third component (Algol C). ... The surface temperature distribution for Algol A­B system before (upper plot) and after (lower plot) correction for temperature due to the irradiation e#ect. ... We solve this equation by the iterative Newton­Raphson method. ...

Еще в разделе: (Показать все результаты (>209) - www.stecf.org/ )

• Introduction

... The Network Time Protocol (NTP) is used to synchronize the time of a computer client or server to another server or reference time source, such as a radio or satellite receiver or modem. ... Information on the NTP architecture, protocol and algorithms can be found in the Further Information and Bibliography page. The Building and Installing the Distribution page presents an overview of the procedures for compiling the distribution and installing it on a typical client or server. ...

Еще в разделе: (Показать все результаты (>1869) - www.sai.msu.su/ )

• Supernovae distribution according to their magnitudes.
• Copyright
• Building and Installing the Distribution

... As of the 95NOV release, patch level 2.0, ESO-MIDAS is available under the GNU General Public License. The short statement of the GNU license is included in every MIDAS file; the full text is printed in the beginning of this manual and is included as a separate file in the ESO-MIDAS Release. ... All source code, documentation, as well as binary copies of ESO-MIDAS (already installed and without sources) for specific systems can be retrieved from the ESO-MIDAS anonymous ftp account. ...

Еще в разделе: (Показать все результаты (>1422) - www.sao.ru/ )

• Noise distributions
• Direct electron imaging-model
• Some statistical trends and distributions

A study of the size and composition of dust grains in the circumstellar envelope of IRC + 10 o 216 S. Bagnulo, J.G. Doyle and I.P. Griffin We utilise a modelling technique in which a generalised two­stream Eddington approximation is applied to the problem of the radiative transfer in a spheri­ cally symmetric dust shell. ...

Еще в разделе: (Показать все результаты (>2039) - star.arm.ac.uk/ )

• Galactic distribution and absolute magnitudes
• Armagh Observatory
• Stellar Atmospheres Software

Stellarium 0.12.3 . ... FileљStructure . FileљList . ... core . modules . Skylight.hpp . ... 33 љ float color[3]; // 3 component color, can be RGB or CIE color system . ... 48 љ void setParams( float sunZenithAngle, float turbidity); . ... 109 љ float zenithLuminance; // Y color component of the CIE color at zenith (luminance) . 110 љ float zenithColorX; // x color component of the CIE color at zenith . 111 љ float zenithColorY; // y color component of the CIE color at zenith . ...

Еще в разделе: (Показать все результаты (>762) - astro.uni-altai.ru/ )

... Big ellipse: the region of the photometric analysis Smaller ellipses: the adopted inner boundaries of the Main Body and the C component Small circles: diffuse background objects, manually selected and removed from the photometry Uncleaned CMDs [V-I, I] of I Zw 18, obtained using Aloisi et al. (left) and Izotov & Thuan (right) datasets. ... Where is the 'halo'? Blue compact dwarf galaxy SBS 1415+435 Hubble Space Telescope / Advanced Camera for Surveys NASA, ESA A. Aloisi (STScI, ESA) et al. ...

Еще в разделе: (Показать все результаты (>228) - mavr.sao.ru/ )

• Measurement of the dark halo shape in polar ring galaxies
• Galaxy sector, archive 2014
• Optical component of GRB080319B

... Give laxation where number a simple order of magnitude argument to show why the retime for 2-bo dy encounters in a stellar system TR 3 /m2 n, is the velo city dispersion, m the typical stellar mass and n the density of stars. (10 marks) 2. From B&T 99, question 2.3). The density distribution (r ) = 4 M rJ 3 4 r J r 2 (r + r J ) 2 (where M and rJ are constants) for a spherical galaxy is called a Jaffe mo del (after Walter Jaffe of Leiden University, who devised it). ...

Еще в разделе: (Показать все результаты (>580) - www.mso.anu.edu.au/ )

• http://www.mso.anu.edu.au/seminars/abstracts/20160301-1100.html
• Siding Spring Survey
• Richard Woolley and Jim Banham inspecting optical and mechanical components,

Last time we saw that flat rotation curves for galaxies, when measured in galaxies with extended gas distributions, provides unambiguous data that shows the mass distribution is dominated by an unseen, spherical halo. ... Perhaps only galaxies with extended dark matter halos are capable of retaining large gaseous extents? . ... Clusters of Galaxies: . ... The case of the Cancer cluster: . ... Below is the velocity distribution of galaxies in the Cancer cluster: . ... What's going on in Cancer? ...

Еще в разделе: (Показать все результаты (>365) - zebu.uoregon.edu/ )

• Current Weather Conditions
• Fossil Fuel Primer

Next: Uncorrelated flux component Up: Introduction Previous: The Hierarchical Stellar Systems Contents . The type parameter allows to select from a range of stellar models, either analytical, or availbale as data files or FITS images. ... For all types from zero to 11, the flux distribution is computed as flat ( teff=0 ), a black body ( teff < 0 ), or a stellar atmosphere ( teff > 0 ). For all types, specifying an arbitrary SED will override stellar spectra or fluxes derived from the images. ...

Еще в разделе: (Показать все результаты (>44974) - www.eso.org/ )

• ESO - ESO-MIDAS Releases and Distribution
• KMOS Exposure Time Calculator
• IAU Symp317 Scientific Program