. Вид изнутри . Древний Аланский храм 9-го века н.э. расположеный на севере . руин аланского городища, в Зеленчукском ущелье около современного . поселка Нижний Архыз . Страница: 2/2 | <<< 1 2 . Сохранившиеся элементы настенной росписи в восточной части храма . Западная часть храма . Вид на прихожую изнутри храма . Вид на прихожую изнутри храма . IMGP1522_a . В прихожей храма . Захоронение . Powered by GRAY , 2006 . Gallery created by FotoAlbum.

Laboratory of Stellar Physics . ... A study of close binaries with black holes, neutron stars and white dwarfs. ... A study of SS433 - the massive close binary with a black hole in the regime of supercritical accretion . ... A search for intermediate-mass black holes (IMBH). The black holes which are not supermassive black holes observed in quasars, and which were formed not in massive stars. ... A search for new magnetic stars, new CP stars, measurements of magnetic fields in stars . ...

... Modernization of the BAO NAS RA 1-m Schmidt Telescope . The modernization of the 1-m Schmidt telescope of the Byurakan Astrophysical Observatory (NAS of Armenia) is finished. ... The results were reported at the international conference "The Present and Future of Small and Medium-Size Telescopes" (SMT-2015), September 19-22, 2015, Nizhny Arkhyz . ... V.Gabrielyan, T.Movsessian, Modernization of the Byurakan Astrophysical Observatory 1-m Schmidt Telescope, SMT-2015 Conference Abstracts, p.36; . ...

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

... Corresponding gates in each row are connected in parallel at both edges of the array. ... Other gates. ... otherwise indicated, 45 kpixels/sec and standard voltages using a dual slope CDS circuit (8 µs integration time) Minimum Format Pixel Size Imaging Area Dark current (MPP), 20° C equivalent Readout noise Front Back Full Well signal Output gain CTE per pixel Typical 512 x 512 pixels 24 µm x 24 µm 12.3 mm x 12.3 mm 50 pa/cm2 5 electrons 7 electrons 350,000 electrons 1.5 µV/ electron 0 ...