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http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt.
http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt.
1. http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt
Title: High-Resolution Near-Infrared Speckle Interferometry and Radiative Transfer Modeling of the OH/IR star OH~ 26.5 + 0.6 Authors: T. Driebe(1), D. Riechers(2), Y. Balega(3), K.-H. Hofmann(1), A.B.\ Men'shchikov(4), and G. Weigelt(1) (1)Max Planck Institute for Radioastronomy, Bonn, (2)Max Planck Institute for Astronomy, Heidelberg, (3)Special Astrophysical Observatory, Nizhnij Arkhyz, Russia, (4) ... 2004, A&A 435, 563), and from L-band observations (Starck et al. ...
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Ссылки http://mavr.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt -- 3.4 Кб -- 05.05.2009
[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt -- 3.4 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt -- 3.4 Кб -- 24.02.2010
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[ Сохраненная копия ] Ссылки http://www.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt -- 3.4 Кб -- 24.02.2010
[ Сохраненная копия ] Ссылки http://jet.sao.ru/hq/balega/PUBL_BAL/PUB_2005/driebe_ag2005_oh26.5.txt -- 3.4 Кб -- 24.02.2010
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2. Armagh Observatory
... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... A sketch for the active region model on ultracool dwarfs. ... An active region model was built, based on the rotation of the UCD and the ECMI mechanism. ... The active region model is applied to the radio emission from TVLM 513-46546, in which the ECMI mechanism is responsible for the radio bursts from the magnetic tubes and the rotation of the dwarf can modulate the integral of flux with respect to time. ...
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Ссылки http://star.arm.ac.uk/highlights/2010/567.html -- 6.8 Кб -- 08.09.2010
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3. HST Focus Model
... Focus Model . ... For a given time, this model estimates the amount of defocus at a particular camera. ... If you obtained focus model values from this site prior to May 23rd, for HST observations made after March 29th 2011, then obtaining those values again now will improve agreement with measurements. ... the average focus value over the time period requested (measured and/or modeled values as applicable). a link to a space-delimited text file containing Date, Julian date, Time, and Model value . ...
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Ссылки http://www.stsci.edu/hst/observatory/focus/FocusModel -- 16.6 Кб -- 10.04.2016
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4. Spatial Structure of NGC 6822: An Example for Statistical Modeling of
... 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 . ...
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Ссылки http://www.adass.org/adass/proceedings/adass94/pasztorl2.html -- 11.0 Кб -- 03.11.2000
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5. The AstroStat Slog Blog Archive [MADS] multiscale modeling
... Archives . ... On the other hand, CHASC scientists relate more general and broad statistical inference problems in estimating the intensity map, like intensity uncertainties at each point and the scientifically informative display of the intensity map with uncertainty according to the Poisson count model and constraints from physics and the instrument, where the field, multiscale modeling is associated. As the post title [MADS] indicates, no abstract has keywords multiscale modeling. ...
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Ссылки http://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/mads-multiscale-modeling/index.html -- 24.9 Кб -- 01.03.2014
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6. INTAS project 2003
... Prof. J. Hough (University of Hertfordshire, United Kingdom) . ... Astrophysics Research and Light Scattering Groups, University of Hertfordshire, UK (6 persons) . Max Planck Institute for Astronomy, Heidelberg, Germany (4 persons) . Sobolev Astronomical Institute, St.Petersburg State University, Russia (5 persons) . Institute of Computational Mathematics and Mathematical Geophysics, Novosibirsk, Russia (5 persons) . ... The site of the previous INTAS project (Open Call 1999 grant 652) . ...
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Ссылки http://www.astro.spbu.ru/staff/ilin2/INTAS2/ -- 6.0 Кб -- 19.11.2010
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7. http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Plucinsky.pdf
Chandra X-Ray Observatory CXC 1. ... E0102: Joint Fits with ACIS S3, MOS1/2 & pn Paul Plucinsky, Joseph DePasquale, & Steve Snowden Paul Plucinsky 1 EPIC Cal April 2007 Chandra X-Ray Observatory 1. ... E0102: Gratuitous Pretty Pictures of E0102 S3 Summed Data ~100 ks CXC RGS Spectrum (Pollock 2006) Objective: develop a spectral model which can be used by RGS, HETG, EPIC & ACIS, etc. ...
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Ссылки http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/200704/Plucinsky.pdf -- 1429.9 Кб -- 13.05.2014
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8. Space Research Institute (IKI) Seminar
... Future seminars . ... G.V. Levina (Institute of Continuous Media Mechanics) . ... Abstract . ... The INTEGRAL mission and its first results" . ... Reconnection - new basic results and solar simulations " . October, 30 . ... D.L. Vainchtein (IKI RAN; Dept. of Mechanical and Environmental Engineering, University of California Santa Barbara, USA) . ... New results on Solar Structure and Dynamics and Solar Space Observatories " . ... E.B. Gliner (Theoretial Research Institute, San Francisco) . ...
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Ссылки http://www.iki.rssi.ru/galeev/english/past2003.htm -- 25.2 Кб -- 09.01.2008
[ Сохраненная копия ] Ссылки http://www.cosmos.ru/galeev/english/past2003.htm -- 25.2 Кб -- 09.01.2008
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[ Сохраненная копия ] Ссылки http://www.cosmos.ru/galeev/english/past2003.htm -- 25.2 Кб -- 09.01.2008
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9. http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf
ON THE IMPACT OF THE GALACTIC ABERRATION ON VLBI-DERIVED PRECESSION MODEL Z.M. MALKIN Pulkovo Observatory Pulkovskoe Ch. ... Corrections to adopted precession rate are usually computed from the linear trends in long-term time series of celestial pole offset (CPO), which are the differences between the measured and the theoretical coordinates of the celestial pole. ... CONCLUSIONS We have estimated the impact of GA on parameters of precession-nutation model derived from VLBI observations. ...
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Ссылки http://www.gao.spb.ru/english/personal/malkin/publ/zm12e.pdf -- 37.3 Кб -- 10.12.2012
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10. Results of recent and ongoing site programs
... Liyong Liu (NAOC) . Site testing on seeing conditions of the astronomical observatories over China are briefly reviewed, including Xionglong station of NAOC, Gaomeigu station of Yunnan Observatory, Delingha station of Purple Mountain Observatory. ... PDF [3.0€аMB] October 8, 09:55 10:20 . ... In this paper, we will review the site survey activities in the past years, and present the site-testing results on the Oma site, including cloud cover, seeing, water vapor, transparency and sky brightness. ...
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Ссылки http://site2010.sai.msu.ru/section/5 -- 6.7 Кб -- 09.04.2016
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11. Radar Meteor Workshop
... Effects of meteor ablation and the chemistry and physics of the upper atmosphere . ... Ablation and Ionization Modeling: Implications for Trail Instabilitiesand Head Echoes . Radar Observations of Meteors at a Polar Latitude . ... Radar meteor shower observations: processing and some results . ... Parameter estimation of meteors from radar head echoes combined with optical observations . ... Observations of meteor-head echoes using the Jicamarca 50 MHz radar in interferometer mode . ...
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Ссылки http://www.naic.edu/~djanches/radarWorkshop/ListOfSpeakers.htm -- 21.4 Кб -- 03.03.2003
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12. Journal "Peremennye Zvezdy"
Peremennye Zvezdy ( Variable Stars ) 35 , No. ... We present the results of our new observations of QS Draconis, a recently discovered double-mode high-amplitude Scuti variable, HADS(B) type. ... Our CCD observations in the Johnson bands were performed at the Tien Shan Astronomical Observatory of the V.G. Fesenkov Astrophysical Institute, at the altitude of 2750 m above the sea level. ... The finding chart (Fig. 1) identifies the variable star, comparison star, and check star. ... Fig. ...
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Ссылки http://www.astronet.ru/db/varstars/msg/1333529 -- 29.0 Кб -- 17.12.1972
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13. Science Innovations
. Сайт временно не работает.
14. Labo J.-V.Poncelet: L.O.Chekhov
Born: March, 29 1962 (Moscow) . ... Inst., ... Inst. in 2001. Title of thesis: "Matrix models and geometry" . ... Courses in theoretical mechanics, field theory, and string theory in the College of Mathematical Physics of Independent Moscow University in years 1994--2001. ... Quantum field theory: gauge and supersymmtric theories, matrix models and integrable systems, graph theory. ... By L.O.Chekhov and R.C.Penner Russ.Math.Surv. ... 7) Matrix models versus Seiberg-Witten / Whitham theories. ...
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Ссылки http://www.mccme.ru/lifr/pers/chekhov.htm -- 6.2 Кб -- 04.10.2006
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15. II. MPDG - Some preliminary results
The problem of eXtremely-Metal Deficient (XMD) galaxy ages. ... Problem of ages of XMD galaxies is addressed through the comparison of colours of stars in their outer regions (where one can neglect the effect of recent star-formation activity), with model tracks of evolving stellar populations from, e.g., the popular package PEGASE.2 (Fioc Rocca-Volmerange 1999). For some of XMD galaxies, the contribution of nebular emission in the light of outer regions is negligible or invisible. ...
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Ссылки http://www.sao.ru/precise/Laboratory/Current/MPDG_r2.html -- 4.3 Кб -- 05.02.2007
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16. ATCA 3mm Recent Results
... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australia Telescope User Committee . ... Australian Square Kilometre Array Pathfinder . ... Parkes radio telescope . Australia Telescope Compact Array . ... Australia Telescope Online Archive (ATOA) . ... ATCA . ... Visiting Australia Telescope Compact Array . ... Parkes radio telescope webcam . ... 3mm Home Page System Performance Calibration Observing Quick Start System Specs mmATCA Receivers mmATCA Results . ...
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Ссылки http://www.atnf.csiro.au/observers/docs/3mm/results.html -- 49.6 Кб -- 08.04.2016
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17. Sternberg Astronomical Institute
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) . ...
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18. Description of the RadioAstron project, english version
Status of the RadioAstron project development . The engineering model of the Space Radio Telescope (SRT) was assembled in Lavochkin Association (LA) in the configuration consisting of 10-m parabolic radio astronomical antenna made of carbon-fiber, F ocal and Device cabins of the scientific payload and on-board and ground complex of high data rate up-down radio link (VIRK). ... Then,radio astronomical tests were conducted using real radio sources. ... Space Radio Telescope . ... Data Processing . ...
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Ссылки http://www.asc.rssi.ru/RadioAstron/description/status_eng.htm -- 7.2 Кб -- 10.05.2008
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19. Bojan Nikolic -- Nested sampling modelling of Star-Formation History of the
... Bojan Nikolic web pages home . ... As an exercise to put through the new InMin library through its paces, I have looked recently at applying Nested Sampling ( Skilling2006 ) algorithm to the fitting of star-formation history as function of redshift. ... The data I used are from Figure 1 of Yuksel08 but I use only the grey data paints, which are just the data originally from Hopkins2006 . ... The next step is to define the function which is the model for the history of the SFR density. ...
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Ссылки http://www.mrao.cam.ac.uk/~bn204/blog/2012/05/22/nestedsampling-sfr-hist.html -- 20.2 Кб -- 05.10.2015
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20. Dust grains from the heart of supernovae
... Staff . ... Cosmic dust has been observed both in emission and extinction everywhere in our Galaxy as well as in many other galaxies. ... Dust grains are classically thought to form in the winds of Asymptotic Giant Branch (AGB) stars. However, nowadays there is increasing observational evidence for notable dust formation in Supernovae (SNe). ... Hence the observed dust mass of 0.7вИТ0.9M вКЩ in this source can be safely considered as indicative of the mass of freshly formed dust in SN ejecta. ...
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Ссылки http://www.arcetri.astro.it/en/home-english/204-scientific-news/1095-dust-sn -- 30.4 Кб -- 10.04.2016
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