... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

Еще в разделе: (Показать все результаты (>1997) - www.adass.org/ )

• Modelling Spectro-photometric Characteristics of Nonradially Pulsating Stars
• Stochastic Relaxation as a Tool for Bayesian Modeling of Astronomical Images
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries

... The perceptron structure, on the basis of which the database is built, is defined by a number of the input and output parameters and a required accuracy. ... The output perceptron data are the expansion coefficients of the scattering matrix elements in series of the generalized spherical functions. ... As the cluster structure depends on the generation conditions the expansion coefficients were averaged over 5--7 realizations of the clusters (for N . ... is the coefficient number. ...

Еще в разделе: (Показать все результаты (>352) - www.astro.spbu.ru/ )

• Vladimir P. Reshetnikov's Home Page
• paper2

ASC-FITS-2.0.1: ASC FITS File Designers' Guide (Rots and McDowell) (1999 Jun) . ASC-FITS-REGION-1.0: FITS region document (McDowell and Rots) (1998 Mar) . ... CXC-DM-001 Introduction: Data Analysis with the Chandra Data Model (2001 Oct) . ... 1998 Feb 26: SDS-1.0: Data Product List: obsolete . ... 1998 Mar 09: SDS-10.0: (ASC-FITS-REGION-1.0) FITS region document: see ASC-FITS-REGION-1.0 . 1998 Feb 09: SDS-11.0: FITS function document (superseded by ASC-FITS-FUNCTION-1.2) . ...

Еще в разделе: (Показать все результаты (>2779) - hea-www.harvard.edu/ )

• Jonathan's ASC documents
• Vertical Structure of the Secondary: Hydrostatic Model
• *fit* - Fit Data to a Specified Model

THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE BY MEANS OF DIGITAL MODELS. ... The surface brightness of Mercury was measured Danjon (1933, 1949, 1953) and Harris (1961) in phase angle 3o-123o. The analysis of the various data of the integral photometric gives the results of determination of the main photometric constants for Mercury. ... THE PHOTOMETRIC RESEARCHS OF THE MERCURY'S SURFACE: S.G. Pugacheva The surface brightness of the Mercurian images was established on the geologic map Mercury. ...

Еще в разделе: (Показать все результаты (>135) - selena.sai.msu.ru/ )

• http://selena.sai.msu.ru/Pug/Publications/ms42/m42_60.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms082.pdf
• Svetlana G. Pugacheva

The dust properties in the Large and Small Magellanic clouds (LMC/SMC) are studied using the HERITAGE Herschel Key Project photometric data in five bands from 100 to 500 m. Three simple models of dust emission were fit to the observations: a single temperature blackbody modified by a power-law emissivity (SMBB), a single temperature blackbody modified by a broken power-law emissivity (BEMBB), and two blackbodies with different temperatures, both modified by the same power-law emissivity (TTMBB). ...

Еще в разделе: (Показать все результаты (>15270) - www.stsci.edu/ )

• Attenuation Effects in Spiral Galaxies: Multiwavelength Photometry and Disk
• Practical Validation of Results
• Results

The Earth's magnetosphere global structure is conditioned by the interaction of the Solar wind and Earth's magnetic field. ... Solar wind (SW) - the region outside BS; . ... Auroral field lines (AUR) region - the funnel-shape cavity restricted by the geocentric distance of the order of 6 RE, between surfaces formed by magnetic field lines emerged from the polar and equatorial OVAL borders; . ... Fairfield D.H., Average and unusual location of the Earth's magnetopause and bow shock, J. Geophys. ...

Еще в разделе: (Показать все результаты (>1459) - www.cosmos.ru/ )

• (Q-6) Expansion of the Bohr Model

... We apply an additional restrictions on the model which follow from recent helioseismic results: 1) calibration of the surface helium abundance and the specific entropy in the convection zone (Vorontsov et al. ... AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA AAAA...

Еще в разделе: (Показать все результаты (>1613) - crydee.sai.msu.ru/ )

• http://crydee.sai.msu.ru/ftproot/pub/local/science/publications/tenerife.94/ten94.ps.gz
• http://crydee.sai.msu.ru/ftproot/pub/local/science/publications/wien.92/wien92.ps.gz
• http://crydee.sai.msu.ru/ftproot/pub/local/science/publications/circ.94/circ94.txt

... Metallic€а nanostructured mesostructures are formed as a result of their self-assembly while growing of nanoclusters and nanowires during the pulsed current electrodeposition process on the membranes. Our work shows that the pulsed current electrodeposition on the templates is a general biomimetic method to fabrication of metal models of natural objects: protozoa, plants, mushrooms, shells. ... тАвThe growth on the€а membranes or templates . ... The layered structure . of the shell . ...

Еще в разделе: (Показать все результаты (>1479) - www.issp.ac.ru/ )

Next: MASSES Up: EXTREME HELIUM STARS: PULSATION Previous: STELLAR PROPERTIES . ... Following main-sequence evolution, a red giant star in a close binary system may expand to fill its Roche lobe. ... Although Iben & Tutukov (1984) used this model to account for the EHes, the latter are not binaries (Jeffery et al. ... Final helium-shell flash in a post-AGB star. ... Accretion from the disk onto the surviving WD creates a star with a degenerate CO core and a helium envelope. ... Other models. ...

Еще в разделе: (Показать все результаты (>2729) - star.arm.ac.uk/ )

• A Blinker Model
• Armagh Observatory Preprint No. 308
• V652HER AND MERGED BINARY WHITE DWARF MODELS

... Numerical Modeling of RadioAstron SRT Temperature Deformations M. Yu. Arkhipov, I. S. Vinogradov, S. B. Novikov, and S. D. Fedorchuk Astro Space Center, Lebedev Physical Institute of the Russian Academy of Sciences, Moscow, Russia e mail: rusengineer@mail.ru Received December 16, 2013 Abstract--The results of modeling the thermal deformations of a space radio telescope's reflecting surface are presented in the paper. ...

Еще в разделе: (Показать все результаты (>160) - www.asc.rssi.ru/ )

• RadioAstron meeting
• Description of the RadioAstron project, english version
• ОТЧЕТ

... Abstract: We present Monte Carlo radiative transfer simulations for spiral galaxies modelled as a stellar disk and a two-phase clumpy dust distribution. ... As a general result, clumpy models are less opaque than the corresponding homogeneous models. ... 0.00 0.15 0.50 0.1 0.5 1.0 2.0 5.0 10.0 0.25 X . ... We have also produced several homogeneous models, to compare to the clumpy models. ... Homogeneous and clumpy models with the same tauV have the same dust mass. ...

Еще в разделе: (Показать все результаты (>6748) - www.arcetri.astro.it/ )

• Atlas of Monte Carlo Models of Dust Extinction in Galaxies

... CentralProcessor 0.11 documentation . Calibration and Imaging Documentation . The cmodel pipeline task is responsible for extracting a local sky model (LSM) from the global sky model (GSM) and building an image from the components and/or images resulting from the request. ... MPI wrapper> cmodel -c config.in . ... None . ... If Cmodel.gsm.database is set to asciitable then a row/column (space separated) file is used as the global sky model source. ... cmodel (Model Image Generator) . ...

Еще в разделе: (Показать все результаты (>15903) - www.atnf.csiro.au/ )

• Unified Radio Catalog: results for Version 1.1
• The Structure of Dark Halos: Model-Independent Information from HI Rotation
• Thin screen scintillation model

... Research . ... Laboratory . Main results . ... webmaster@izmiran.ru . The main results of the research are: . From the Cosmos-1809, Intercosmos-19 and Cosmos-900 satellite data the ring ionospheric trough, RIT, associated with the ring magnetospheric current and SAR-arcs was revealed and its characteristic were in detail investigated. ... C) 2007, IZMIRAN ...

Еще в разделе: (Показать все результаты (>558) - www.izmiran.rssi.ru/ )

• IZMIRAN - Laboratory for Physics and modeling of the ionosphere
• IZMIRAN: Laboratory for Physics and modeling of the ionosphere - publications -

Еще в разделе: (Показать все результаты (>416) - lnfm1.sai.msu.ru/ )

• Trudy GAISH, vol. LXV, 1996, Abstracts in English

The Model of The Distribution of SNe in a Spiral Galaxy. ... In this article we represent the model of the distribution of SNe of the II type in the disk of a spiral galaxy. ... No.1557 ­4 0 4 8 0 20 40 60 I­ exp disc II­ 1/r disc III­ II type SNe IV­ All SNe III IV I II Radius, kpc. Log s. Radial distribution of SNe. 0 0.2x10 4 0.4x10 4 0.6x10 4 0.8x10 4 1.0x10 4 ­5.0 ­2.5 0 2.5 5.0 Delta R, kpc Number of SNe ­ Delta R ###. ...

Еще в разделе: (Показать все результаты (>768) - xray.sai.msu.ru/ )

• The Model
• ADS Abstract Service Results
• Seminars

Next: Fit routines Up: Basic widget procedures Previous: Load data Contents . The following menu bundles all routines related to reading and fitting of the hierarchical model. The fit routine should not be confused with specialized and customized fitting routines to be found elsewhere (in AMOEBA FIT). ... C ALC Compute model data. FIT General model fitting widget. ... The general model fitting widget displays all components of the model, and the parameters associated with each one of them. ...

Еще в разделе: (Показать все результаты (>66121) - www.eso.org/ )

• Model manipulation
• Gaitee Hussain @ ESO
• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations

My research interests are focussed on the theory and modelling of accretion processes as well as star and planet formation mechanisms. I am particularly interested in the stability properties of accretion discs, the generation of MHD turbulence and associated angular momentum transport, disk - planet interactions and the origin and characteristics of jets and winds from accreting systems . ... These results have been published in Salmeron & Wardle, 2005, M.N.R.A.S., 361: 45-69. ...

Еще в разделе: (Показать все результаты (>713) - www.mso.anu.edu.au/ )

• Towards a Truly Unified Model of AGN
• Giant Galaxy String Defies Models of How Universe Evolved
• Marc White - Astrophysicist - The Australian National University

Abstract . A self-consistent model for the dynamical and chemical evolution of dense interstellar clouds is examined. The model includes the basic atomic and molecular constituents of dense clouds and the reactions in which they are involved. ... The results of one-dimensional modeling of the early stages of collapse of protostellar clouds of different masses under the action of ultraviolet radiation are presented. Astrophysical applications of the results obtained are discussed. ...

Еще в разделе: (Показать все результаты (>43) - www.inasan.rssi.ru/ )

• chemazh

... Models of central engines (1) Potential of disk accretion onto stellar mass black holes: disk binding energy: thin disk life time: - accreted mass - disk outer radius - gravitational radius - Shakura­Sunyaev parameter Ultra-dense Hyper-Eddington neutrino cooled disks !! ... 1989); Neutron star + Neutron star Neutron star + Black hole White dwarf + Black hole Black hole + compact disk Burst duration: 0.1s ­ 1.0s Released binding energy: (1.2) Collapsars­ origin of long duration GRBs? ...

Еще в разделе: (Показать все результаты (>951) - www.iki.rssi.ru/ )

• Magnetic field models[Oulu]
• IKI - MSR Research Workshop
• Substorm models [Oulu]

We have designed the laboratory model of static Fourier spectrometer for onboard usage for spectral study of atmosphere and ionosphere. The gain of model is to simulate onboard FS which will not have any moving elements (all its optical elements will be mounted at fused quartz monolithic construction), to compare experimental results with theoretical estimations and to measure MTF of CCD array. ... This fact connected with low frequency response of CCD array due to small format of it. ...

Еще в разделе: (Показать все результаты (>98) - space.univ.kiev.ua/ )

• Theoretical Astrophysics
• Solar Physics
• Optical static Fourier spectrometer