. Comment on J0126-0123 . No detection: this object has been studied with the Molonglo telescope at 408 MHz (Schilizzi & McAdam 1975) as a source with a size between 2 and 5 . It is near an Abell cluster (Owen & Ledlow 1997). The data could be confused with a strong radio source (3C 40) identified with a pair of galaxies at z=0.018, 170" from our field center. VLBApls home page . Last modified: 16 Oct 2000

... Contact A Problem of an estimation of accuracy of the asteroid CCD observations . The Minor Planet Center supported by the Interntional Astronomical Union is the main office for keeping observational data of the small Solar System bodies and their investigations. ... At Pulkovo Observatory we are estimating an accuracy of the CCD asteroid observations obtained by amateurs and professional astronomers all over the World using the MPC database. ...

RADIOASTROPHYSICAL DEPARTMENT • INSTITUTE OF SOLAR-TERRESTRIAL PHYSICS RAS SB . Research results on fast active processes General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases ... Distribution of the recorded spikes in duration . ...

... Seminar archive . ... Титарчук Л. X-ray spectral index correlations vs mass accretion rate in neutron star and black hole X-ray binaries in their different spectral states. ... vs mass accretion rate as in the case of NS as well in the BH case. In BHs the spectral index should increase and then saturate with mass accretion . ... BH case the index, indeed, correlates and then saturates with mass accretion . rate. Moreover this index-mass accretion rate correlation allows us to estimate . ...

... part 1 | ... The Basic Stages in Earth's Pre-geological Development . ... After fragments of the Vortex sleeves separated, whirlwinds of second and third orders ("NC" - new micro-vortex) were generated- future planet cores and their satellites - all of them developing independently, governed by the common laws of development of cosmogenic vortexes. ... Our planet's core today is comprised of considerably deteriorated cosmogenic vortex; consequently, the Earth has a moderated magnetic field. ...

. Institute Structure . • Administration . • Research Divisions: . Superhigh energy particles . Space plasma physics . Aeronomy . • Center of information technology . • Stations: . Yakutsk Extensive Air Shower (EAS) Array . Polar Geocosmophysical Observatory (PGO) . Complex Geophysical Station (CGS) . Optical Station . Yakutsk Cosmic Ray Spectrograph . Magnetic Observatory . Ionospheric Station . Station for Receiving of Satellite Information .

Астрономия и Космос Небесные тела Черные дыры и пульсары . А строномы получили наблюдательные подтверждения того, что некоторые черные дыры вращаются вокруг своей оси , подобно водоворотам. ... Следовательно, черные дыры , как и нейтронные звезды, могут вращаться вокруг своей оси . ... Комментарии к Черные дыры вращаются вокруг своей оси . Ссылки по теме Черные дыры вращаются вокруг своей оси: . Черные дыры вращаются вокруг своей оси . Черные дыры и пульсары . Имитация черных дыр . ...

. Main . Final stage of OC "MIR" flight . Photoarchives . RUSSIAN AVIATION AND SPACE AGENCY . CENTRAL SCIENTIFIC RESEARCH . MACHINE BUILDING INSTITUTE . MISSION CONTROL CENTER . Russian . Earth Orbiting Complex "Mir" . The material submitted to the UNO Science and Engineering Subcommittee 38 session on peaceful use of space (Vienna 12-13 Feb 2001) as an oficial UNO document . Press-conference at MCC February 28, 2001, U.N. Koptev

... Luna-9 lander . ... Luna-16,20,24 return capsules . ... Luna-16 drill . Luna-16 drill cutaway . Luna-16 drill base . ... Luna-17 . Luna-17/21 closeup . Luna-17/21 ramp . Luna-17/21 top view . Luna-17/21 bottom view . ... LK landing leg shock absorber . ... LK engine . Krechet detail . Krechet lunar suit . ... Venera-8 lander . ... VEGA TV platform . Venera-2..-7 engine . ... VEGA lander . ... Vega baloon probe . ... Mars/Venera engine . ... Mars-3 lander . ...

. General Information . Media Files . Participants . Timetable . Local Information . Photos . October 5, 15:00 15:30 . Victor Kornilov (SAI) . PDF [2.4б MB] October 5, 15:30 16:10 . Florian Kerber (ESO) . PDF [2.0б MB] October 5, 16:10 16:35 . Boris Safonov (SAI) . PDF [704.7б KB] October 5, 16:35 17:05 . October 5, 17:05 17:45 . Pavel Kovadlo (ISZF), Olga Kochetkova (ISZF) . PDF [4.0б MB] October 5, 18:20 19:00 .

... However, our studies show that Prosilica EC650 has very good p erformance to use as DIMM image detector. ... The sub-directories /opt/dimm/data/out for the output data file, /opt/dimm/data/log for the output log file yymmdd-dimm.log and /opt/dimm/etc for the configuration file must b e created. ... Pictures mode The Pictures mode provides grabbing of the star b ox images and storing their sequence as one output file "b oxrecord.fits" in /opt/dimm/data/images/ sub directory. ...

Добро пожаловать, Гость . ... Общероссийская неделя "Астрономия на тротуаре" - 15-17 апреля . ... Астрономия и общество (Модераторы: ivanij , Oleg Tuchin ) ? Награда для любителей астрономии . ... Гость . ... Белый Дом, США: Палата Представителей одобрила в среду 3 марта законопроект, предложенный Комитетом по Науке, согласно которому астрономам-любителям за обнаружение околоземных астероидов будет выдаваться вознаграждение размером 3 тыс. долл. ... Записан . ... Ответ #1 : 05.03.2004 [21:42:47] ? ...

... Twenty-Six Year Monitoring of Water Masers IAU Symposium 242, Alice Springs 1 Contents of the work A sample of H2O maser emission sources has been observed since 1980. ... Rudnitskij et al. ... Twenty-Six Year Monitoring of Water Masers IAU Symposium 242, Alice Springs 4 Maser in a protoplanetary disc (S255) Flux density, Jy S255: H2O line profile 5 February 2002 Radial velocity, LSR, km/s Rudnitskij et al. ... Twenty-Six Year Monitoring of Water Masers IAU Symposium 242, Alice Springs 12 ...

VISTA Data Flow System: Status Jim Emerson*a, Mike Irwinb, Nigel Hamblyc b a Astronomy Unit, Queen Mary Universit y o f London, Mile End Road, London E1 4NS, UK Inst itute of Astronomy, Universit y of Cambridge, Madingley Road, Cambridge CB3 0HA, UK, c Inst itute for Astronomy, School of Phys ics, Universit y of Edinburgh, Edinburgh EH9 3HJ, UK ABSTRACT Data from two IR survey cameras UKIRT's WFCAM and ESO's VISTA can arrive at rates approaching 1.4 TB/night for of order 10 years. ...

... Р?С?С?С?Р?Р?Р?Р?РеС?Р?С?Р?РеР? ... Launched on February 17, 1996, the Near Earth Asteroid Rendezvous (NEAR) mission is to be the first of NASA's Discovery missions, a series of small-scale spacecraft designed to proceed from development to flight in under three years for a cost of less than $150 million. ... The ultimate goal of the mission is to rendezvous with and achieve orbit around the near Earth asteroid 433 Eros in February, 1999, and study the asteroid for approximately one year. ...