Contents. planet: 5 - Jupiter satellites: J1 - Io : 10, J3 - Ganymede : 15, J4 - Callisto : 6 total number: 31 type: relative dates: 1997-1997 observatory: see observatories list in the relevant article. ... Emelianov N. V., Vashkovjak S. N. (2009) Astrometric results of the observations of the mutual occultations and eclipses of the Galilean satellites of Jupiter in 1997. ... Position angle A in degrees (topocentric for mutual occultation or heliocentric for mutual eclipse) 10. ...

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• jg0036
• jg0025
• jg0028

... Fig. 1a,b. Location of slit spectrograms on the HА-line image of IC10. ... Relative abun dances Relative abundances of oxygen are derived using three methods. ... Figures 2, 3, 4 show the distributions of the inferred 12+log(O/H), log(N/O), log(S/O) values along the slits; we averaged the abundances over HII re gions from the catalog of Hodge and Lee [5]. ... Relative oxygen abundance along the slits. ... Relative nitrogen abundance along the slits. ... Relative sulf ur abundance along the slits. ...

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Spectropolarimetry and modeling of Galactic Wolf-Rayet star WR156 O LGA M A RY E VA Special Astrophysical Observatory RAS; olga.maryeva@gmail.com For the first time spectropolarimetric observations of Wolf-Rayet star WR156 (WN8h sub-class) were conducted. ... This polarization is, most probably, has an interstellar origin, as its magnitude and orientation are similar to the ones of field stars. ... By its parameters WR156 is similar to other WN8h stars, displaying the line effect. ...

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• Principal scientific results
• LSFVO: Results
• GRB follow-up team

... If done carelessly this can cause a never-ending loop. However as a programming technique it is often used to simplify such tasks as searching down through a directory tree. a text pattern consisting of a combination of alphanumeric characters and special characters known as metacharacters . ... See UNIX File System for a more detailed explanation. any host on the network which you are not presently using. the directory located at the top of the Unix file system. ...

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• Multiwavelength Study of Mira Ceti-Type Variable Stars
• Captions

... A document window is shown, with 8 lines (numbered 1 to 8), each 24px high. The text of the "outer" box (at the end of line 1, halfway into line 2, and halfway into line 3) is shifted upward 12px. The text of the "inner" box, thought shifted upward as well, has been relatively positioned so that it lies in its normal flow position at the end of line 2. ... The lines, as they appear in the image, contain: Start 1 Beginning of body contents. 2 of outer contents. Inner contents. ...

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• Dynamic HTML in Communicator
• Frequency/duration relation.
• Long description for example illustrating positioning with respect to a

... The ROSAT Consortium (the Max-Planck-Institut fuer extraterrestrische Physik, the Goddard Space Flight Center, the Smithsonian Astrophysical Observatory, Leicester University, and the Astrophysikalisches Institut Potsdam) announces the release of the completed source catalogs of all ROSAT pointed observations. ... Detailed information about the catalog and methods of access to the catalog and data products can be obtained from the ROSAT Results Archive web pages in Germany, in the US, and in the UK:...

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• Cool Stars 10 - J.U. Drake and V. Kashyap: Coronal Metallicity of HR 1099
• ChaMPlane data_archive_.html
• The AstroStat Slog Search Results google sky

... The first column shows the kinematical diagrams, where is the angle between the line of sight on the object and the vector of rotation about Z -axis, and V S is objects line-of-sight velocity relative to an observer at rest at the position of the Sun. The straight lines are regression fits, whose slopes yield the subsystem’s rotation rate. The second column shows the relations between metallicity and distance from the Galactic plane. ... privious figure | next figure . ...

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• Mid Scales Role
• Vertical Structure, figures
• Vladimir Marsakov Abstracts

... Julian Date Flux Densities (mJy) Julian Date Flux Densities (mJy) 2440000:0 A1 A2 B C 2440000:0 A1 A2 B C 8930.9968 153.8 134.6 59.8 22.6 9021.6846 154.0 137.0 59.0 22.9 8939.7717 163.7 146.0 66.1 22.9 9024.6766 151.4 134.6 58.4 22.1 8940.8936 153.2 135.8 59.2 22.6 9030.5334 156.7 139.1 59.0 22.4 8944.7380 161.7 142.2 63.7 23.1 9032.6650 151.8 136.5 57.7 22.6 8951.8637 148.4 131.3 58.3 21.7 9036.7067 155.1 137.1 58.8 ...

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. Yu.A.Shokin . Accurate positions of variable stars in the western part of the Large Magellanic Cloud bar . (published in IBVS and SAI Proceedings ) . B.S.Vozdvijenski, N.P.Gorbatko, V.A.Yeliseev, G.V.Romanova . The results of the observations of the selected minor planets in Sternberg State Astronomical institute . (published in SAI Proceedings ) .

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PULSE PROFILES AND CYCLOTRON LINE ENERGY DEPENDENCE ON X-RAY PULSARS LUMINOSITY S. Tsygankov, A. Lutovinov, E. Churazov, and R. Sunyaev Space Research Institute, Profsoyuznaya str. ... CYCLOTRON LINE ENERGY 2.1. ... We concentrate on the luminosity and energy dependence of the pulse profile and the variations of the cyclotron line energy. In V0332+53 the line energy changes nearly linearly with the source luminosity, while in 4U0115+63 its behavior is more complicated. ...

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• SIXA acceptance tests, 2000
• Zeldovich-100 / International Conference / Moscow, Russia
• Sergei Grebenev, Home Page

... Maps of six sources (0420+022, 0420-014, 1308+326, 1345+125, 1803+784, and DA 193) obtained with milliarcsecond resolution are presented and discussed, together with their broadband (1­22 GHz) spectra obtained on the RATAN­600 radio telescope at epochs close to those of the VLBI observations. ... The image (Fig. 5) shows that the source structure at 18 cm is compact, consisting of a VLBI core and two jet components, with the outer component lying 5 mas (30 pc) to the northwest of the core ( = 54 ). ...

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• http://astra.prao.psn.ru/SUB/abstract2006.htm

... GCR and SCR are primary cosmic rays. 10-15 years after the discovery of cosmic radiation (1919) there emerged two main avenues of investigation in the physics of cosmic rays (CR): 1) nuclear - elucidation of the origin of elementary particles and nuclear interactions; and 2) astrophysical (space physics) - solution of the problem related to the origin and variations (changes in intensity) of CR. ... Besides, the CR flux in interplanetary space is, strictly speaking, not isotropic. ...

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Berlin, Germany . Berlin was founded in the early thirteenth century as the capital of Brandenburg. ... After the Second World War, the city was partitioned into East and West Berlin. ... Though medical and educational facilities were well funded in both East and West Berlin, housing remained a problem for both. Inadequate housing retarded the population growth of East Berlin, and West Berlin suffered from the destruction of one third of its housing to during the Second World War. ...

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• Центр образования г.Зеленогорск :: Проекты:: Results
• results

... www.chjaa.org or http:/ / /chjaa.bao.ac.cn ) Chinese Journal of Astronomy and Astrophysics A Check on the Variations of Earth's Rotation with an Ancient Solar Eclipse Yan-Ben Han and Qi-Yuan Qiao National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012; hyb@bao.ac.cn Received 2003 May 13; accepted 2003 September 29 Abstract We address the relation between an ancient total The total eclipse was recorded in some ancient Chinese books, especially in local chronicles. ...

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• Jovian GRS longitude
• Stellarium: ScreenImage Class Reference
• Jupiter

... Стайлер Блоу Даун крим Разглаживающий крем благодаря антистатическому действию масла Ши обеспечивает гладкость волос надолго! . ... Линейка: Total results Mega Sleek . ...

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• Original Xiaomi Mi Position Activated Carbon Filter Кардиган длинный
• Lenovo c20-30 19.5", Белый, 4Гб, 500Гб, DOS, Intel Celeron - Lenovo - Lenovo
• Органайзер для косметики El Casa "Цветы", цвет: синий, красный, белый, 23 х 23

... Reports on progress and error are always recorded in the log file of the program. ... UT date of the measurement finish in YYYY-MM-DD format UT time of the measurement finish in hh:mm:ss format Average flux in A aperture Average flux in B aperture Average flux in C aperture Average flux in D aperture Normalized variance of flux in A aperture Normalized variance of flux in B aperture Normalized variance of flux in C aperture Normalized variance of flux in D ...

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• atmos 3.0 page

The purpose of the space-physics lab exercises is to introduce the students to the methods of the measurements, to the modern conception of near-Earth space structure and the physical processes and phenomena occured in it. ... At present the reasearches and the teachers of the University and of other institutes participating in the project continue development of the the special space-physics lab exercises, and they are interested in your ideas concerning the future exercises. ...

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• University Satellites and Space Science Education '2006

J E N A M - 2000 Moscow . ... We are pleased to confirm that the JENAM-2000 meeting will take place in Moscow, Russia, in May 29 - June 3, 2000. ... Registration form . ... You can submit it through the Web-page (highly desirable) URL: http//www.inasan.rssi.ru/INASAN/JENAM . ... Please, visit JENAM-2000 Web-pages http://www.inasan.rssi.ru/INASAN/JENAM , http://www.sai.msu.su/jenam , http://www.aip.fr/eas/meetings.htm for news and additional details about JENAM and associated events planning. ...

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• Спец.выпуск N5 (октябрь, 1999).
• Выпуск N6, декабрь 1996

... About Space Monitoring Laboratory, scientific directions, instruments, contacts . ... Optical afterglow GRB030329 (first image in Europe - 5 h after GRB) . ... GCN Circ 11231 | ... 26 sec after Notice time. ... GRB 100319A ( GCN 10527) - 64 sec after Notice time and 78 s after the GRB time. ... GRB 091127 ( GCN 10203) - MASTER early optical transient polarimetry We see bright OT! 9 sec after Notice time. ... GRB06011A ( GCN 4485 )- Optical limit 16.0 130 s after the GRB time 130 s after the GRB time...

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• Ya.B. Zeldovich All-Moscow Seminar of Astrophysicists
• International Workshop ?Robotic observatories?

Crater Gassendi . ... I made this drawing was made on the 26th of november 2001. If you compare this one with the previous drawing of Gassendi (below) the differences are clear. ... This drawing was made on the 28th of september 2001. After nearly a full month without observations I had a one hour gap between the thicker clouds. ... This drawing was made on the 29th of august 2001. ... This drawing was made on the 27th of august 2001. ... This drawing was made on the 25th of august 2001. ...