... A Chemically Decoupled Nucleus and Inner Polar Ring of the SBb Galaxy NGC 4548 O. K. Sil'chenko* Sternberg Astronomical Institute, Universitetskii pr. ... This nucleus, a probable circumnuclear disk coplanar with the global galactic disk, is embedded in the bulge whose stars are generally also young, T 4 Gyr, although they are a factor of 2.5 more metalpoor. ... O. K. Sil'chenko, Pis'ma Astron. ... It remains to assume that the gas at the center of NGC 4548 rotates in an inclined plane. ...

... At the January meeting we finally achieved the necessary quorum in the vote on the bylaws changes proposed in September. ... Giant Ribbon at Edge of the Solar System: Mystery Solved? ... It is where solar wind particles heading out into interstellar space are reflected back into the solar system by a galactic magnetic field." ... Particles from the solar wind that escape the solar system are met ~100 astronomical units (~15 billion kilometers) away by an interstellar magnetic field. ...

... Родился 24 октября 1954 года в городе Сторков (Storkov), Германия. ... С 1980 по 1981 год учился в аспирантуре в психофизиологической лаборатории Физиологического Института Университета им. 'Фридриха Шиллера' (Psychophysiological laboratory at the Physiological Institute of the Fr.Schiller University) в городе Йена по проблеме вызванных потенциалов (evoked potentials). ... С 1992 по 1995 год работал в Центре молекулярной медицины им. 'Макса Делбрюка' в Берлине. ...

... Our scientific interest is an accuracy of asteroid CCD observations obtained by amateurs and professional astronomers all over in the World. ... These data help us to analyse an accuracy of real CCD positions in the MPC Database. ... Do you test your observations of the small Solar System bodies permanently before sending them to the International Minor Planets' Center? ... Do you know a real accuracy of your positional CCD-observations in comparison with the other observatories' one ? ...

... ARTICLE: The Adventurous Search For The Astronomical Unit . ... Kepler himself had suggested to use the rare occasions of Venus transiting (crossing) the solar disk to measure our distance to the planet. ... Due to the orbital inclination of Venus against the ecliptic of 3.5°, a Venus transit is so rare that it happens only at intervals of 121.5 years, 8 years, 105.5 years, 8 years and so on. ... Crabtree witnessing the transit of Venus 1639 . ... Transits of Venus - The Quest for the Solar Parallax...

... Миссия "Cassini - Huygens" (NASA и ESA) . ... Хронология за 2004-2006 года . ... Close (altitude = 2,100 km; 1,300 mi) of moon . ... Distant (altitude = 68,000 km; 42,000 mi) of moon . ... Cassini passage through plane [South to North] (160,000 km; 100,000 mi wrt ) . ... Closest distance (78,000 km; 49,000 mi) to on rev number 0 . ... Distant (altitude = 107,000 km; 67,000 mi) of moon . ... 01/03/2005 . ... Closest distance (211,000 km; 131,000 mi) to on rev number 3 . ... Start rev number 3. ...

... 1596, 2013 February 13 The Solar Corona: Why It Is Interesting for Us Abstract. Strong magnetic fields are of vital importance to the physics of the solar corona. They easily move a rarefied coronal plasma. ... They change geometry of magnetic field. ... First, we apply the concept of fast reconnection of electric currents as the source of energy for microflares to explain coronal heating in quiet regions (Somov B.V. and Hґ enoux J.-C., in Magnetic Fields and Solar Processes , 9th Eur. ...

The monitoring of the optics quality of DIMM instrument V. Kornilov, B. Safonov May 24, 2010 1 Intro duction A quantitative theory of measurement of optical turbulence (OT) with Differential Image Motion Monitor (DIMM) is based on certain priori assumptions [1]. ... Bottom: behavior of the instrumental Strehl's number for the left (triangle to the left) and right (triangle to the right) DIMM images during the period of measurement the maintenance of an additional correction factor seems superfluous. ...

The 2dF QSO Redshift Survey (2QZ) . ... Before jumping into all the finer details of teh survey, a brief non-astronomer's guide to redshift surveys is available. ... The primary scientific aims of the QSO survey are: (1) to obtain the primordial fluctuation power spectrum out to COBE scales, (2) to determine the rate of QSO clustering evolution in the non-linear and linear regimes and hence obtain new limits on the value of and the bias parameter, (3) to apply a powerful geometric method to measure . ...

Хранение ультрахолодных нейтронов в магнитной ловушке из постоянных магнитов. ... Прецизионное измерение времени жизни свободного нейтрона (n в экспериментах при низких энергиях имеет принципиальное значение для физики элементарных частиц и космологии. ... Для используемой геометрии ловушки для эффективной очистки спектра через нижний барьер требуется не менее 400 с. Использование магнитного хранения УХН для измерения времени жизни нейтрона имеет одну замечательную особенность. ...

... Роман Евгеньевич Ильинский email : ilinsky_r@mail.ru . ... Ильинский Р. Е., Ровенская Т. С. Дифференциалы луча в оптической системе // Вестник МГТУ. ... 1998.- ... Roman Ilinsky , Gradient-index meniscus lens free of spherical aberration, Journal of Optics A: Pure and Applied Optics, volume2, number 5, pages 449-451, year 2000 . ... Ильинский Р. Е. Определение реальных габаритов пучков в градиентных оптических системах // Прикладная оптика -2000: Тез. докл. ... 2000.- ... ROMAN ILINSKY . ...