... Abstract: We present an extensive study of the radiative transfer in dusty galaxies based on Monte Carlo simulations. ... We have explored the dependence of A_l on a conspicuous set of quantities (Hubble type, inclination, dust optical thickness, dust distribution and extinction properties) for a large wavelength interval, ranging from 1250A to the K band, thus finally providing a comprehensive atlas of dust extinction in galaxies, which is electronically available. ... S04_MD20[ att , abs ] . ...

... We find a transition of LBV star from the LBV instability strip to the region of classical WN for the first time. ... Numerical modeling of the atmospheres of these objects are very important for understanding the evolutionary relationship WR and LBV stars, as well as of the physical causes of LBVs variability. We studied spectra of two very luminous stars in the M33 galaxy - LBV V532 and late WN star FSZ35. ... Bottom: The spectrum of FSZ35 with the final model . ...

... This method is based on putting space modules, vehicles and EVA-suit donned cosmonauts in the swimming pool under conditions of neutral buoyancy, indifferent equilibrium and unsupported state. ... You can also dive into the swimming pool with the SCUBA equipment in order to examine the mock-ups of space stations and vehicles and pass a course of rehabilitation in a hyperbaric oxygenation complex. ... Services / Hydrospace: General description Technical description "Orlan" suit Photo gallery Price . ...

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... Model . ... Karpachev A.T., IZMIRAN, e-mail: karp@izmiran.ru . ... To the Model: . The empirical median model of the shape and position of the MIT (Main Ionospheric Trough) in the Northern and Southern Hemispheres is presented. ... Geomagnetism and aeronomy, v.26, № 1, p.63-68, 1986. ... Karpachev A.T., Afonin V.V. Dependence of the ionospheric trough occurrence probability on the season, local time, longitude, and level of magnetic activity Geomagnetism and aeronomy, v.38, № 3, p.79-91, 1998. ...

. This Directory contains Model of distribution of density, temperature and effective collision freguency of electrons. Yu.K.Chasovitin. 1998. This Directory contains The program RIM98 for calculating the parameters of the ionosphere to use the "Reference Ionospheric Model-98" (RIM-98).Yu.K.Chasovitin. 1998.

... I am involved in Project Astro, a program to bring astronomers into public schools to assist with teaching students about science and astronomy. ... While there are all sorts of scale model of the Solar System type exercises ( Mitchell Charity's page has a good listing of what's available), none were really tailored towards discovering the spatial relationships of the planets, and in a way that could be done at night as part of a Star Party. ...

... reference to the following paper: Karakas Lattanzio (2007, PASA, submitted) Each file contains: 1) pulse number 2) the core mass , Mcore ( Msun ) 3) maximum mass of the intershell convection zone, M_csh ( Msun ) 4) duration of intershell convection , t_csh (years) 5) mass dredged into the envelope, D_dredge ( Msun ) 6) lambda 7) lambda_dup defined by Goriely Mowlavi (= lambda x (DMh/Mpulse) where Mpulse is the maximum ...

... Forum . ... Recent Topics . ... MAO main . ... Fw: School-Seminar БЂњModeling of . ... Sent: Monday, June 23, 2014 4:28 PM . Subject: School-Seminar БЂњModeling of physical processes in condensed matterБЂќ . ... in condensed matter (M3PhysProc)БЂќ ( . ... October 2014 (Sumy, Institute of Applied Physics NAS of Ukraine, see . ... The school-seminar topics are theoretical and experimental physics of . ... test.mao.kiev.ua/images/postbyemail/M3PhysProc-poster_2014.pdf . ... MAO NASU . 2014 ...

... Different equations of state tables can be used, including SAHA-S equation of state. ... 1) separate input fields for X and Z are used, each line contains only T and rho; example: 2.17e6 0.18 . 2) each line contains T, rho, X and Z; separate input fields for X and Z are ignored; example: 2.17e6 0.18 0.74 0.018 . 3) each line contains T, rho, X, Z(CNO), Z(Ne), Z(FeSi); separate input fields for X and Z are ignored; example: 2.17e6 0.18 0.74 0.010 0.002 0.006 . ...

... Артикул: A-6164N Цвет: розовый Состав: 80% полиэстер, 20% вискоза Уход за изделием: стирка при 30њС Страна дизайна: Турция Страна производства: Турция Товар сертифицирован. ... Объем: 1.7 л; Мощность: 2200 Вт; Тип нагревательного элемента: закрытая спираль; Материал корпуса: пластик . Цвет: белый . ... Артикул: PL000028AW1 (FRIDA) Цвет: черно-молочный Состав: 94% вискоза, 6% эластан Описание: Идеально стройнящее фигуру платье, комбинированное эластичным итальянским трикотажем и батистом. ...

... The most powerful and widely used methods to calculate the scattering matrix of a fractal cluster are based on the coupled dipoles methods (e.g. the Discrete Dipole Approximation, DDA) and the theory of light scattering by a cluster of spherical particles [2-4]. ... At present the procedure of calculation of the scattering matrix is well developed for both an oriented cluster of spherical particles and for chaotically oriented clusters of such particles [4]. ...

Modeling of atmospheres of the brightest stars belonging to the Cyg OB2 association O LGA M A RY E VA , V. G . K L O C H K OVA , E.L. C H E N T S OV Special Astrophysical Observatory RAS; olga.maryeva@gmail.com We present the results of modeling of the spectrum of the brightest stars belonging to the Cyg OB2 association ­ Cyg OB2 #7 (O3If ) and Cyg OB2 #11 (O5Ifc). ... The lines in Cyg OB2 #7 spectrum are divided into three groups which can not be described with a single model. ...

Next: Initial binary parameters Up: Population synthesis of Previous: Introduction . Monte-Carlo method for statistical simulation of binary evolution was originally proposed by Kornilov & Lipunov (1983a,b) for massive binaries and developed later by Lipunov & Postnov (1987) for low-massive binaries. ... Recently Leitherer & Heckman (1995) have modelled star formation for elliptical and spiral galaxies, taking into consideration only the single stars. ... Initial binary parameters . ...

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... G., Filippova A.S. Presented by: Filippova A.S Achievements · Refined model based on the celestial-mechanics methods is presented that is a generalized version of the previously developed basic model · Subtle effects are qualitatively explained based on the amplitude-frequency analysis and the computer numerical modelling of the oscillatory pole motion, where the key feature is the Chandler wobble 2 Basic Model of the Polar Oscillations ...

... 8, ``Celestial Mechanics'', 2002 High--accuracy modelling of the Earth's gravitational potential from GOCE satellite gradiometry mission M. S. Petrovskaya, A. N. Vershkov Pulkovo Observatory, St. Petersburg, Russia The Earth's gravitational potential is presented in form of a spherical harmon­ ic series with the coefficients C n;m which are the fundamental dynamical constants for the Earth. The set of C n;m for degree 0 џ n џ N and order jmj џ n consti­ tutes a geopotential model. ...

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... LX90 Series . MeadeтАЩs LX90 ACF is a favorite of astronomers making the jump to their first, serious, larger aperture telescope. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... Coronado Accessories . ... LX90 GPS Module (8" models) . ... LX90 GPS Module. ...

Общая Астрономическая Конференция > Товары для астрономов > Полезное для астрономии . Solar Model 1.2 . ... Поиск . Сообщения за день . ... falerg . ... Сообщений: 17 . ... Отметил для себя интересную программу Solar Model 1.2. ... Описание: Solar Model 1.2 - позволит вам путешествовать меж планет, контролировать ход времени, наблюдая ускоренное или замедленное движение небесных тел (планет, лун, астероидов). ... Solar Model 1.2 - Скачать . ... Отправить личное сообщение для falerg . ...

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. ...