... Родился в 1947 году в городе Сеттл (Settle) в церемониальном графстве Северный Йоркшир (North Yorkshire) на севере Англии. ... В 1971 - 1975 годах работал в штате Гринвичской астрономической обсерватории (Royal Greenwich Observatory). С 1975 году работал в отделе астрофизических исследований (Astrophysics Research Division) Калемской лаборатории (Culham Laboratory), расположенной возле города Абингдон (Abingdon) в графстве Оксфордшир (Oxfordshire). ... Был женат на Кейт Пэтчетт (Kate Patchett). ...

... Flight Engineer of Soyuz TMA . ... He began astronaut training in February 1984 and served as backup payload specialist to Marc Garneau for the October 1984 space shuttle mission STS-41G. Dr. Thirsk has been involved in various Canadian Space Agency projects including parabolic flight campaigns and mission planning. ... He is currently training in Russia to serve as the backup crewmember to European astronaut Roberto Vittori for the April 2005 Soyuz 10S taxi mission to the International Space...

... GEORGE GAMOW . ... George Gamow had the true Odessa temperament, his scientific ingenuity and cheerful humor were inexhaustible. ... In 1994, in the year of his 90-th anniversary, an International Conference "Astrophysics and cosmology after Gamow" was held in Odessa and St.Petersburg. ... In 1999, in the year of his 95-th anniversary, an International Conference " The universe of Gamow: original ideas in astrophysics and cosmology " was held in Odessa and St.Petersburg. ...

1972, May 23 born in Mannheim / Germany . ... 1994-1998 studies in physics at the University of Heidelberg / Germany . ... 1998 degree Diplom-Physiker diploma thesis at the Landessternwarte in Heidelberg . ... 1999-2002 Ph.D. thesis about the simulation of jets of highly redshifted radio galaxies in Max Camenzind's group at the Landessternwarte in Heidelberg . ... 2002-2004 Postdoc in Max Camenzind's group at the Landessternwarte in Heidelberg . ... This page is maintained by Martin Krause ...

... Telescopes . ... 1993: . ... For the first time a device for quasi-simultaneous measurements of linear polarization of stars was developed, which allows to make up to 40% more efficient the use of the telescope time and significantly increase its accuracy. ... Fast systems of high spectral resolution were developed and put into operation at the 6-m BTA and 1-m Zeiss telescopes, consisting of the echelle spectrometers, solid-body light detectors (CCDs), data acquisition and data processing systems. ...

In the regular experiments carried out with the RAS radio telescopes at Pushchino during 1999-2002, the study of the radial dependence of scattering of compact natural radio sources was extended to remote regions of the solar plasma environment. ... The stream in the transalfvenic region displays the same typical radial structure as observed in the transonic region, i.e., the existence of a "precursor" - a narrow band of reduced scattering preceding a wide region of enhanced scattering. ...

Krasnoyarsk, Russia . We live in Siberia- the region in the centre of Russia. Our city is called Krasnoyarsk. ... Our city is located on the . ... We are students of secondary comprehensive school number . ... There are about 700 children aged from 7 to 17 at our . school. We are in the 8th form We teach English and would . ... and very often walk to the most beautiful place of our city . ... Our best regards to everybody. postal address: . ... Russia . 660095 . ...

. Prague, August 16, 2006 . Present classification : Suggested: . CW, CWA, CWB CW (period will also be given) DSCT, DSCTC, SXPHE DSct (amplitude will also be given, population membership is not always obvious) . L, LB, LC L, Lb (for red stars) . M M . PVTEL PVTel . RR, RRAB, RRC, RR(B) RR, RR0, RR1, RRB01 . RV, RVA, RVB RV, RVb (if the secondary wave's . amplitude is at least equal to that of . the main oscillation) . PULSATING VARIABLES (CONTINUED)

Target: NGC436 Date: 2012-08-22 Time: 06:39 Telescope: CDK20N Camera: Apogeen U16M Filters: g06:39riz Exposure time: 100s per filter Observer: John Kielkopf Processing: John Kielkopf Color map i->R, r->G, g->B square root stretch Lunar scattered light Light dewing of secondary makes a halo on some stars Incomplete compensation of bad CCD column

. Gas density maps that correspond to just before and after the orbit of a secondary supermassive black hole enters the disk of the primary galaxy. Ohio Supercomputer Center

... 78.0, THAT GIVES FOR 27 MONTH (2011, MARCH) DEVELOPMENT CURRENT 24 CYCLE OF SOLAR ACTIVITY THE SMOOTHED MONTHLY MEAN SUNSPOT NUMBER W*mar.= ... 133.8 --------------------------------------------------------------------------- Weekly Bulletin on Solar and Geomagnetic Activity Highlights on 26.09 - 02.10.2011, Forecast on 03 - 10.10.2011, Carrington Rotation 2115 (22,71.09.2011) SOLAR SUNSPOT ACTIVITY OF THE SUN OF THE LAST PERIOD KEPT AT THE CONFIDENT AVERAGE LEVEL. ...

... The CDS bibliographical map is a tool for organizing astronomical text documents into a meaningful map for exploration and search. ... This network contains two layers of nodes: an input layer, and a mapping (output) layer in the shape of a two-dimensional grid. ... The number of nodes is equal to the number of attributes associated with the input. ... The mapping nodes are initialized with random numbers. ... At the end of the training of a map, the number of documents assigned to each node is...

... SEARCH ASP SITE: Match ALL words Match ANY word . ... Astronomy Beat . ... World Beat: Poland . ... For 40 years, the largest Polish planetarium (22 meters), in the southern city of ChorzУw, has been conducting a national Astronomical Olympiad for secondary-school students. ... The larger planetariums offer summer astronomy courses or regular conferences for the physics teachers of their provinces. In recent years, the Polish Astronomical Society has organized workshops for physics teachers. ...

... All the galaxies are divided into 4 groups depending on the environment type; every subsample contains more than 10 galaxies. ... An effect of environments is seen both for the nuclei and for the bulges: if we consider the clusters (Virgo and Ursa Ma jor) and group centers as dense environments and the field and group periphery as sparse environments, then in the dense environments the stellar populations of S0s are in average older by 4­5 Gyr than in the sparse ones. ...

FF Aqr DW Period is significantly greater than typical value for DW type. According to Pojmanski [45] this star is DCEP-FU: variable. According to Sipahi et al. [263] it is one of the few binary systems which consists of the hot subdwarf and cool chromospherically active giant components. ... Belongs to long-period RS CVn systems, secondary is more massive and more larger (volume of the secondary is approximately 100 times larger than that of the primary component). ... So may be SA system? ...