SAI 175 anniversary . ... Moscow University . Search for in SAI Moscow University Search for in Russian astronomical resources . ... SAI Astronomical Databases . ... Browse SAI Software archive(ftp.sai.msu.su) . ASTRONET.RU - Russian Astronomical Network (available in translit also) . ... SAI Supernovae Research Group . ... Department of the Galaxy and Variable Stars (in Russian) . Sternberg Astronomical Institute Seminars . ... All-Russian Astronomical Olympiad (in Russian) . ...

Еще в разделе: (Показать все результаты (>3295) - www.sai.msu.su/ )

• SAI Supernova catalog
• SNe related preprints

Next: Identification and Analysis of Binary Star Systems using Probability Theory . ... We present a computing code for modelling energy flux distributions, photometric indices and spectral line profiles of (non-)radially pulsating Main-Sequence stars. ... In the case of slowly rotating stars one can use the zero-rotation approximation to describe stellar pulsations. Such a model was used already by Cugier, Dziembowski & Pamyatnykh (1994) to study nonadiabatic observables of Cephei stars. ...

Еще в разделе: (Показать все результаты (>1917) - www.adass.org/ )

• Modelling Spectro-photometric Characteristics of Eclipsing Binaries
• Preface
• Distributed Software for Observations in the Near Infrared

... 1 Space Research Institute, Moscow, Russia . ... Classic concept of magnetic merging is represented by pair of flux tubes originating from two interacting magnetic fields reconnected at X-line. This type of reconnection between interplanetary magnetic field and magnetospheric magnetic field received very substantial confirmation from observations. ... We use Interball-Tail observations of ion velocity distributions within magnetospheric boundary layer as tracers of magnetic topology. ...

Еще в разделе: (Показать все результаты (>1425) - www.cosmos.ru/ )

... The department was founded in late sixties by Prof. D.Ya.Martynov, who for many years was also the director of Sternberg Astronomical Institute. At present time, the head of the department is Prof. A.M.Cherepashchuk, a pupil of D.Ya.Martynov and his successor as the director of SAI. Since Prof. Martynov, the scientific activity of the department was primarily related to binary stars. ... The department consists of 15 members most of which have Ph.D. in Astrophysics. ...

Еще в разделе: (Показать все результаты (>29) - uranus.sai.msu.ru/ )

... ATNF Home . About ATNF . ... About ATNF overview . ... Australia Telescope Steering Committee . ... The Hб  I Column Density Distribution Function at z =0: the Connection to Damped Ly Statistics . ... We present a measurement of the Hб  I column density distribution function [ ] at the present epoch for column densities . These high column densities compare to those measured in damped Ly lines seen in absorption against background quasars. ... The Column Density Distribution Function . ...

Еще в разделе: (Показать все результаты (>15710) - www.atnf.csiro.au/ )

• Finding the Bivariate Brightness Distribution of galaxies from an HI selected
• Star formation and gas distribution in the Magellanic Spiral NGC 4214
• An HI selected sample of galaxies -- The HI mass function and the surface

... Jane Charlton, The Pennsylvania State University . Modes of Star Formation and Nuclear Activity in an Early Universe Laboratory . Abstract . ... The Nature of the Halos and Thick Disks of Spiral Galaxies . ... In the coming week, observations are scheduled of OB associations in the M33. ... The present program is combining high-resolution, multi-colour HST imaging with ground-based low-resolution VLT/Keck spectroscopic observations of over 50 strong lensing systems. ... Past weeks: . ...

Еще в разделе: (Показать все результаты (>16976) - www.stsci.edu/ )

• Zolt Levay, Space Telescope Science Institute
• HST this week: 141
• HST this week: 282

... 1 Figure 1: The density distribution in R­Z plane Figure 2: The luminosity distribution in R­Z plane for Maxwellian kick velocity (75 km/s) 2 Figure 3: The luminosity distribution in R­Z plane for Maxwellian kick velocity (150 km/s) n(R; Z) = nHI + 2 \Delta nH2 nH2 = n 0 \Delta exp џ \GammaZ 2 2 \Delta (70pc) 2 – If 2kpc џ R џ 3:4kpc, then nHI = n 0 \Delta exp џ \GammaZ 2 2 \Delta (140pc \Delta R=2kpc) 2 – ; For R џ 2kpc n(R; Z) was assumed to be constant: n(R ! ...

Еще в разделе: (Показать все результаты (>842) - xray.sai.msu.ru/ )

• Old neutron star distribution in the Galaxy
• ADS Abstract Service Results
• Be/X-ray binaries and candidates

... We are using Canadian Galactic Plane Survey l 74.2њ, -3.6њ < b This poster gives preliminary results for a full-fledged analysis of the gas properties and distribution of HISA features in the CGPS. ... where T ON and T OFF are observed brightnesses on and off the HISA feature, T S is the spin or excitation temperature of the HISA gas, tau is its optical depth, T C is the continuum intensity, and p is the fraction of H I emission lying behind the HISA feature. ... GIF | ...

Еще в разделе: (Показать все результаты (>4080) - www.naic.edu/ )

• HISA Poster for the 33rd Annual Meeting of CASCA, May, 2002
• HISA Poster for the 195th Meeting of the AAS, January, 2000

Еще в разделе: (Показать все результаты (>2) - aberrator.astronomy.net/ )

Our publications in 2001 year Kniazev, A. Y.; Engels, D.; Pustilnik, S. A.; Ugryumov, A. V.; Kniazeva, T. F.; Pramsky, A. G.; Brosch, N.; Hagen, H.-J.; Hopp, U.; Izotov, Y. I.; Lipovetsky, V. A.; Masegosa, J.; Marquez, I.; Martin, J.-M. Astronomy and Astrophysics, v.366, p.771-787 (02/2001) . ... Pustilnik, S.; Kniazev, A.; Lipovetsky, V.; Ugryumov, A. Astronomische Gesellschaft Abstract Series, Vol. ... N.; Soboleva, N. S.; Temirova, A. V. Astronomische Gesellschaft Abstract Series, Vol. ...

Еще в разделе: (Показать все результаты (>1435) - www.sao.ru/ )

• MRAO: 7C
• Distribution Policy
• IRAS IDS

... We present centimeter and millimeter interferometric continuum and molecular line images of the massive star-forming region AFGL 5142. ... The emission peak coincides with a 1.5 mJy centimeter continuum source. ... CH3CN (14-13) and (12-11) spectra indicate a gas temperature ~65 K in the innermost core. While the millimeter continuum emission is probably mostly due to optically thin thermal emission from dust grains, the centimeter continuum source is consistent with an ionized wind. ...

Еще в разделе: (Показать все результаты (>8473) - www.arcetri.astro.it/ )

• G35.20-1.74 (Abstract)
• The BD+40 region (Abstract)
• Doug Johnstone's Orion Page

Trudy GAISH, vol. LXV, 1996 . Abstracts . The global distribution of average (5 O x 5 O ) depths . of Mohorovicic discontinuity on the Earth . ... Such analysis allows detecting whether the sources of the largest anomalies reside within the Earth's core. This is possible if the limit depths of the sources exceed the depths of the core-mantle boundary. ... by Pasinok S.L. Influence of the Earth’s cover on the polar free oscillation of the Earth’s inner core is considered. ...

Еще в разделе: (Показать все результаты (>393) - lnfm1.sai.msu.ru/ )

• My Links

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Quasi-stationary electron distributions for the different values of the particle escape time. ... The electron-cyclotron maser instability is widespread in the Universe, producing, e.g., radio emission of the magnetized planets and cool substellar objects. ... The model used takes into account the radiation escape from the source region and the particle flow through this region. ...

Еще в разделе: (Показать все результаты (>2462) - star.arm.ac.uk/ )

• Atmospheres
• Nuffield Science Bursaries at Armagh Observatory
• Southern African Large Telescope (SALT)

... 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 (>1514) - www.mrao.cam.ac.uk/ )

• Inference of Coefficients for Use in Phase Correction
• Astrophysics Group Opening of Battcock Centre for Experimental Astrophysics
• Paper I: Method Bojan Nikolic web pages (r. 329)

Еще в разделе: (Показать все результаты (>359) - zebu.uoregon.edu/ )

• Radiation Dominance in the Early Universe
• U of O High Energy Physics Seminars
• Astronomy HyperText Book: Stellar Clusters

Magnetic stars, 2004,225-229 Averaged magnetic phase curves. ... ANALYSIS OF THE CATALOG 227 4 3 N stars 2 1 -4000 -3000 -2000 -1000 0 1000 2000 B0 (G) Figure 3: Number distribution of stars vs. coeffcient B0 for those stars which exhibit a magnetic phase curve with a double wave. of a magnetic star can occur if the angle between the magnetic and rotational axes is small or even zero. ... The catalog lists phase curves for 139 stars, 134 of them are magnetic Ap stars. ...

Еще в разделе: (Показать все результаты (>981) - jet.sao.ru/ )

• http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2006/riechers_etal_oh104.9+2.4_eso05.pdf
• Spectral energy distribution

Microsymposium 34, MS059, 2001 A HIPSOMETRICAL FEATURES OF THE LUNAR SURFACE FROM THE CLEMENTINE MISSION. ... The lack of extensive mare basalt fill in the South Pole ­ Aitken Basin, despite the thin crust in this region, suggests hemispheric compositional asymmetry in the deep lunar interior [1]. ... According to new data, the depths of Mare Imbrium, Mare Frigoris, Mare Fecunditatis, Mare Moscoviense are 0.5 km deeper than previous results indicated. ... 1994) The Clementine Mission to the Moon. ...

Еще в разделе: (Показать все результаты (>130) - selena.sai.msu.ru/ )

• http://selena.sai.msu.ru/Rod/Publications/ms34/MS060.pdf
• http://selena.sai.msu.ru/Rod/Publications/ms38/ms035.pdf
• http://selena.sai.msu.ru/Pug/Publications/Pugacheva%20LPS%2041.pdf

... Graduated from Moscow State University in 1970 and till now in permanent staff of the Sternberg Astronomical Institute, Moscow State University. ... Member, Euro-Asian Astronomical Society . ... Jointly with Dr. V.Konnikova, I teach a course in Radio Astronomy at the Astronomy Division , Physics Department of Moscow State University . ... Astronomical Meetings . ... Net Search: MetaCrawler . ... Moscow State University . ... Rudnitskij, Georgij M. Page last updated November 25, 2015. th . ...

Еще в разделе: (Показать все результаты (>168) - comet.sai.msu.ru/ )

• Instructions for Authors
• Hot links of Comet WWW site

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 (>6862) - xmm.vilspa.esa.es/ )

• Null-hypothesis probability distribution for a weighted sum of Poissonian
• Distribution of colours

... 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 (>238) - www.stecf.org/ )

• http://www.stecf.org/conferences/adass/adassVII/reprints/daszynskaj.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/grochevae.ps.gz
• http://www.stecf.org/conferences/adass/adassVII/reprints/gamielk.ps.gz