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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• SAI SN RESEARCH GROUP

. [ Go back to Comet WWW site ] . Andrew A. Martis . martis @ sai.msu.ru .

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... Keith S. Noll, Space Telescope Science Institute . Binaries in the Kuiper Belt: Probes of Solar System Formation and Evolution . Abstract . ... HST FUV Observations of Brightest Cluster Galaxies: The Role of Star Formation in Cooling Flows and BCG Evolution . ... Optical and Ultraviolet Photometry of Isolated Neutron Stars . ... GO 11113: Binaries in the Kuiper Belt: Probes of Solar System Formation and Evolution . A composite of HST images of the Kuiper Belt binary, WW31 . ...

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• HST this week: 064
• STIS Instrument Handbook
• Chapter 7: Observation Strategies

Peremennye Zvezdy", . ... 10, N 26 (2010) . ... Star Name: . ... We report an increase of the J-band brightness of the unique supergiant FG Sge by the summer of 2010. It follows from our IR observations of the star (1986-2010) that its J-band brightness level in August, 2008 reached an absolute minimum (~12 m ), and till the beginning of the summer of 2010, the star was almost inaccessible for observations at 1.25 microns. ... The figure shows J-filter brightness variations of FG Sge in 1986-2010. ...

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A team of U.S. and German astrophysicists have made the first ever detection of X-rays coming from a comet. ... Following the initial detection, the team reported repeated X-ray emissions from the comet over the next 24 hours. ... One preliminary theory is that X-ray emission from the Sun was absorbed by a cloud of gaseous water molecules surrounding the nucleus of the comet, and then were re-emitted by the molecules in a process physicists call "fluorescence." ... Comets . ...

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• Space Research Institute (IKI) Seminar

Lab . Main page News People . ASA . Master . Master net Homepage . ... Lomonosov Moscow State University Sternberg Astronomical Institute . ... MASTER . ... Lomonosov (ShOK) . ... About Space Monitoring Laboratory, scientific directions, instruments, contacts . People, who work in lab . Latest news and news archive . ... All news ...

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... 2000: . According to the BTA observations, the redshift Z=0.7063+-0.0017 was measured for a distant galaxy possessing the 24 magnitude, in which there occurred an explosion of a massive star, followed by a gamma-ray burst catalogued as GRB991208. ... In collaboration with the Space Telescope Science Institute (USA), the Institute of Astrophysics of Andalusia (Spain). ... According to the Palomar Sky Survey, about 600 new nearby dwarf galaxies were discovered. ... Archive . ...

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• Galaxy sector, archive 2004
• Galaxy sector, archive 2012
• Detection of unique bright radio flare of X-ray binary

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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• Intelligent Life in the Universe
• U of O High Energy Physics Seminars
• Astro-2 and the UIT Experiment

... It is found that the correlation coefficients between these two parameters calculated separately inside and outside the sunspot formation zone ±30 have cyclic variation and occur in anti-phase. This suggests different mechanisms of formation of the corona in the fields of small, medium, and large scales. ... The relationship between the coronal green line brightness (CGLB) and the magnetic field strength (MFS) has been investigated by constructing the corresponding synoptic maps for the 1977-2001. ...

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... It provides long range planning information to the scheduling team; it provides bright object, timing, and orientation information to the observation planning team; and it provides graphical description of the observations and their constraints. ... The GUI graphically displays the constraints that are computed by Spike and stored in the description files and in the database. ... BOAS processes all bright objects that have entered the database since the last time BOAS was run. ...

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• Classification of Objects in the Guide Star Catalog
• Restoration of HST WFPC2 Images in Gyro-Hold Mode

Институт Космических Исследований . ... Физика планет и малых тел Солнечной системы . ... Федеральное государственное бюджетное учреждение науки Институт космических исследований Российской академии наук (ИКИ РАН) - головной академический институт по исследованию и использованию космического пространства в интересах фундаментальных наук. ... Одиннадцатая ежегодная конференция "Физика плазмы в солнечной системе" . ... ФГБУН Институт космических исследований Российской академии наук (ИКИ РАН) . ...

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• Space Research Institute (IKI) Seminar

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Lightcurve of HW Vir from images obtained using the Faulkes Telescope South, operated by Las Cumbres Observatory . The blue triangles show the difference between two stars whose brightness is constant. ... This shows the value of the Faulkes Telescopes in the follow-up observations of eclipsing binaries with the aim to detect and characterise additional circumbinary companions. ...

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• Coronal Bright Points: Another Oscillating Environment
• Armagh Observatory
• Explosive Events

... LMC Project Outline . NGC 1818 Initial Results . ... The Large Magellanic Cloud (LMC) is uniquely suitable for the study of massive star clusters at all stages of evolution. By combining HST observations of these clusters with N-body models we hope to understand the origin and evolution of rich star clusters in our own Galaxy, in the LMC, and beyond. ... We aim to combine our HST observations with N-body models to understand the formation and evolution of globular clusters. ...

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• HST NICMOS Observations of Circumstellar Matter Around CYG X-3

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. ...

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• http://selena.sai.msu.ru/Symposium/ir_luna_e.pdf
• http://selena.sai.msu.ru/Bus/Publications/m44_14_busarev_etal.pdf
• http://selena.sai.msu.ru/Shev/Publications/ms38/ms083.pdf

... В четверг, 14 апреля 2016 г., состоится семинар кафедры астрофизики. Повестка дня . ... Начало в 11 час.15 мин. Ауд. ... В четверг, 31 марта 2016 г., состоится семинар кафедры астрофизики . ... В четверг, 24 марта 2016 г. , состоится семинар кафедры. ... В четверг, 17 марта 2016 г. , состоится заседание кафедры. ... ОСП НИИ ПММ Национального исследовательского Томского государственного университета) . ... Copyright 2016 Астрономия в Санкт-Петербургском университете . ...

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• INTAS project 2003
• A Nature of Polar-Ring Candidate Galaxy ZGC 2315+03

The Small Libration of the Satellite in the System of the Asteroid 39 Laetitia . ... Very Long Baseline Interferometry (VLBI), Near Earth Objects (NEOs), near-Earth asteroids (NEAs), small libration of the satellite , Asteroid 39 Laetitia , Crimean astrophysical observatory (CrAO), to automate the observation process, method of frequency analysis , periodicity of changes of asteroid brightness, binary asteroid , binary system , period of axial rotation of components, a satellite ...

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• Keywords_133
• IPA RAN
• Values of asteroid masses

... A1972 Date Received: 2004-Jun-01 13:53:14 Technical Page Proposal Type: Regular General Category : Astronomy Sub- Category : Spectroscopy Observation Category : Extragalactic Total Time Requested: 33 Hours Proposal Title: A Search for Massive Low Surface Brightness Galaxies ABSTRACT: Gaining a rm understanding of Low Surface Brightness ( Observations show increasingly that the `traditional' view of LSB galaxies as low mass, blue young dwarf-like systems is actually incorrect. ...

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• http://www.naic.edu/vscience/schedule/tpfiles/O'NeiltagA1366tp.ps
• http://www.naic.edu/vscience/schedule/tpfiles/AlakoztagV2732tp.pdf
• http://www.naic.edu/vscience/schedule/tpfiles/LewistagA2619tp.pdf

... The R , I photometric observations of SBS 0335-052W were obtained occasionally during the study of SBS 0335-052 with the 3.5m telescope in Calar Alto on 1991 October 6. ... Aperture photometry was performed on the standard star observations using MAGNITUDE/CIRCLE task with the same aperture for all stars. ... For photometry of extended objects, we used the package SURFPHOT as well as dedicated software for adaptive filtering developed at the Astrophysical Institute of Potsdam (Lorenz et al. ...

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• A 10-GHz Radio Continuum Survey
• The Spectrophotometrical complex in Nasmyth-1 focus
• H I 21 cm observations and data reduction

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• Project SUBMILLIMETRON

... Professor of the Moscow University, . Soros professor . New project: MASTER - Mobile Astronomical Systems of the TElescope-Robots. ... Drawing Books Scientific arts Colleagues Teaching . The Best City Vita Painters Fiction New Drawing . Recent popular papers . ... Recent review: . 1.P OPULATION SYNTHESIS OF HIGH ENERGY TRANZIENTS: . FORMATION AND MERGING OF RELATIVISTIC BINARIES( Roma, 1997) . ... lipunov@sai.msu.ru . Send! Send to galja rar . ...

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• Seminars