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... According to the current estimates, a few percent of Main Sequence B5-F5 stars reveal strong surface magnetic fields reaching the values of tens of kilogauss, which is an order of magnitude greater than the maximal magnetic field in sunspots. ... An important direction in the study of magnetic stars is the study of binary and multiple systems with magnetic components using the techniques of spectroscopy and high angular resolution interferometry. ...

... Solar System . ... Planets . ... Until V774104 was discovered Eris (illustrated in this artist?s impression) was the most distant observed member of the Solar System. ... V774104 hardly rolls off the tongue, but this is just a provisional designation and this little world will probably receive a name eventually. ... This bleak little world was found by astronomers led by Scott Sheppard and Chad Trujillo using the 8m Subaru telescope in Hawaii and the Dark Energy Survey Camera in Chile. ...

... In 1930, Trumpler noticed that linear diameters (LD) of open clusters increase with distance (D) from the Sun. ... Since that time, the interstellar absorption has become one of the best studied factor in astrophysics, and we may hope that current OCL distance scales are free from this LD-D correlation. To verify if this is the case we have chosen several modern OCL distance scales and test them with the same clusters and the same angular diameters that Trumpler had used back in 1930. ...

The idea behind it was rather simple: using CGI scripts as processing tools and WWW browser as user interface, display the structure and content of typical anonymous FTP server in a convenient, easily navigated form. ... File Juggler version 1.0 has been implemented and is now installed on two ftp servers at Sternberg Astronomical Institute, Moscow University: . crydee.sai.msu.ru archive (mostly OS/2 software, recreation and leisure) . ...

Name Last modified Size Description . Parent Directory - Artemyev.ppt 03-Mar-2010 19:17 1.6M Frank_IKI-2010.ppt 03-Mar-2010 19:17 5.0M Lyahov.ppt 03-Mar-2010 19:17 1.5M Malova_OFN_2010a.ppt 03-Mar-2010 19:17 5.9M O_Ming_OFN_10.ppt 03-Mar-2010 19:17 14M Petrukovich.ppt 03-Mar-2010 19:17 3.7M Zelenyi_et_al_OFN-2010-v3.ppt 03-Mar-2010 19:17 1.8M .

Name Last modified Size Description . Parent Directory - 98-apogee.rules 2010-06-19 02:22 130 Apn.h 2011-08-03 22:59 7.8K ApnCamera_USB.cpp 2010-06-19 02:17 25K ApogeeUsbLinux.cpp 2011-08-04 01:05 40K README 2011-08-03 23:48 1.6K install_apogee_usb 2010-06-19 15:14 352 libapogeedrv.cpp 2011-08-06 17:19 4.3K libapogeedrv.h 2011-08-06 17:12 833 makefile.xmccd 2010-06-19 02:23 1.5K models.mak 2011-08-03 23:29 4.1K . Apache/2.4.6 (Linux/SUSE) Server at www.astro.louisville.edu Port 80

... What is the configuration of the device driver software? ... If the software you use doesn't adequately tell you what's wrong (or automatically configure it correctly) then you need to investigate how your hardware devices and their drivers are configured. ... Another problem is that when you view configuration messages on the screen, it's sometimes not clear whether the reported configuration is that of the device driver, the device hardware, or both. ...

. Секция «Солнце» . Предварительная повестка дня . Пятница,   29 мая . 14:00–14:15 А. И. Подгорный, И.М. Подгорный.   Солнечная вспышки – модель и сравнение с наблюдениями. 14:15–14:30   Ю .В. Думин , Б.В. Сомов. Топологическое инициирование быстрого магнитного пересоединения . 14:30–14:45 П.А.   Грицык ,   Б.В. Сомов. Модель толстой мишени с обратным током и современные наблюдения солнечных вспышек. 14:45–15:00 Н.П.   Колесников, С.И. Безродных, Б.В. Сомов. Расчет течений плазмы в приближении сильного

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... Protoplanetary Disks and the Hunt for the Youngest Exoplanets . ... Thursday, Apr 14, 2011 at 8:00 PM . ... But associating the current exoplanet properties with their formation epoch can be problematic, since the formation process is intimately associated with the physical conditions associated with their birthplaces: the disks of gas and dust that orbit young stars. ... Apr . ... Copyright (c) Amateur Telescope Makers of Boston, Inc. ...

JANUARY, 2003 . ... FEBRUARY, 2003 . ... MARCH, 2003 . ... APRIL, 2003 . ... MAY, 2003 . ... JUNE, 2003 . ... JULY, 2003 . ... AUGUST, 2003 . ... SEPTEMBER, 2003 . ... OCTOBER, 2003 . ... NOVEMBER, 2003 . ... DECEMBER, 2003 . ... Data archive . ...

... 9) Oknyanskij V.L. 1994, "Optical-radio time delays in Q0957+561", Odessa Astronomical Publ., ... 11) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", in Proceedings of Int. Conf. ... 1994. 12) Oknyanskij V.L. 1994, "Connection between X-ray and optical variability in NGC4151", Astrophys. and Space Science, 222, p.157. ... 14) Oknyanskij V.L., van Groningen E., 1997, "Optical spectral variability of NGC4151 in 1990", Astronomical and Astrophys. ...

For use of "Richland Astronomical Society members only". ... Board index . ... Members . ... This board has no forums. ... In total there are 2 users online :: 0 registered, 0 hidden and 2 guests (based on users active over the past 5 minutes) . Most users ever online was 108 on Sat Jun 09, 2012 9:18 pm . Registered users: No registered users . ... Total posts 254 Total topics 15 Total members 56 Our newest member MichaelMcCoy . ...

This section of library contains information about "classic" Star Catalogs. ... For a Henry Draper Catalog 272149 stars have received a total of 531,211 identifications in 7 сatalogs: . 270456 - in Astrographic Catalogue ( "Carte du Ciel", 4M), . 251943 - in Guide Stars Catalog (GSC), . ... A file with information on the components of 1788 of multiple systems in catalog HDEC (3681 component, or a combination thereof, with 4054 recording). ... A file with information about 21971 variable stars. ...

NASA JOHNSON SPACE CENTER ORAL HISTORY PROJECT BIOGRAPHICAL DATA SHEET NAME: Carl B. Shelley O RAL H ISTORY: 14 April 2001 8 November 2001 CE: BIR M TH DATE/PLA 11 December, 1938 ­ Headland, AL ARITAL STATUS EN : Married to Susan (Somers) CHILDR : Michael (1965); Deborah (1968); Pamela (1973) ESIDENCE: CURRENT R Houston , TX EDUCATIONAL BACKGROUND: B.S. in Electrical Engineering, Auburn University, Auburn, AL, 1960 Graduate work, University of ... Shelley, Carl B. and V. Groom. ...

The XV_VTDF is a viewer for TDF format files (extension to TIFF 6.0 format for storage of high-resolution satellite data). More information about TDF format and relevant topics, as well as satellite data in this format you may receive from Space Monitoring Information Support lab (Space Research Institute, Moscow, Russia) . ... XV_VTDF <filename> - load TDF file at startup (default size) . ... The XV_VTDF operates with fixed-size satellite images in TDF format. ... Back to SMIS Home Page . ...

... S.P. KOROLEV ROCKET AND SPACE CORPORATION ENERGIA . ... OAO RSC "Energia" . ... Company's History . ... History . Brief History of Rocket and Space Technology . ... Flights Chronology . ... ISS Russian Segment . ... A main feature of the series of spacecraft for developmental testing of the interplanetary vehicle is that they will be delivered to ISS on-board Progress spacecraft to be assembled by the space station crew. Contribution of RSC Energia to the Russian Rocket-Space Technology . ...

Альтернативный форум . Scientific.ru Все форумы . ... Hyperboloid (@) - 19.03.2008 18:29 . ... x203a; x203a; x203a; в ответ на: Re: 1994 IAU File of Current Best Estimates Уникум . ... Abramyan G.L., 16.03.2008 13:22 . ... Re::О различии между гравитационной постоянной и гауссовой гравитационной постоянной Уникум, 19.03.2008 14:20 . Re::О различии между гравитационной постоянной и гауссовой гравитационной постоянной Abramyan G.L., 19.03.2008 16:47 . ... Уникум, 20.03.2008 12:47 . ...

UPPER PANEL: The gas surface density map in log scale. The red circle in the center represents the central protostar. The development of spiral structure in the protostellar disk is evident. Dense protostellar/protoplanetary clumsp form within the spiral arms and are driven into the protostar by the action of gravitational torques. LOWER PANEL: The mass accretion rate onto the protostar as a function of time. The mass accretion rate is characterized by very short ( . ...