... The picture shows a 2-dimensional sketch of the outflowing wind of a quasar (Elvis 2000, Astrophysical Journal , vol.545, p.63-76). In the funnel-shaped disk wind Elvis (2000) model a wind arises from a restricted range of radii on the accretion disk around the central black hole. Initially the wind makes a large angle to the disk plane (and so is roughly cylindrical). ... Looking through the quasi-cylindrical part of the wind we see UV and X-ray warm absorbers. ...

This home page belongs to small group of scientists working at . Sternberg Astronomical Institute which is a part of Moscow State University . ... Электронная библиотека научно-технической и художественной литературы (доступна только из ГАИШ) . ... Local staff . Dr. Edward Kononovich (konon -at- sai.msu.ru), Associate Professor . ... Dr. Sergey Ayukov (asv -at- sai.msu.ru), Research Fellow, Webmaster of the group . ... Joint seminar of Solar Studies Structure Group and Solar Photometry Group . ...

... Primordial theory review : Dick Bond . Defects and the CMB review : Andy Albrecht . ... Gravitational wave contribution to CMB anisotropies : V.B. Lukash and E.V. Mikheeva . C_l from cosmic strings : Lloyd Knox . Some aspects of CMB anisotropies induced from topological defects : Mairi Sakellariadou . ... CMB anisotropies from scaling sources : Ruth Durrer . ... SZ observations I : Sarah Church . ... Holes in the microwave sky? ... Detecting cosmic strings in the CMB : James Robinson . ...

... We studied the ionization and thermal structures of the absorption-line systems of quasar spectra. We calculated ionization and thermal structures for several models by varying the density and size of the absorption systems and the intensity and spectrum index of the ionizing spectrum. ... We adopt the photo-ionization model as absorption systems. ... We studied the ionization and thermal structures of the absorption-line systems of quasar spectra based on photo-ionization model. ...

... Mokhovaya st., 11, Moscow, 103907, Russia. ... July 15-17, 1999 , pp. 161-164 . A method for multiple access using the structure of the unstable periodic orbits of chaotic attractor is proposed. Possible principles of the control and selection of unstable cycle-codes are presented. ...

... ATNF Home . ... About ATNF overview . ... Australia Telescope Steering Committee . ... Australian Square Kilometre Array Pathfinder . Murchison Radio-astronomy Observatory . ... Parkes radio telescope . Australia Telescope Compact Array . Mopra radio telescope . ... So far we assumed a homogeneous, steady disk structure. ... We then expect rather inhomogeneous disk structure full of blobs, spots, or filaments, if viewed with X-rays from its vicinity (just like the X-ray image of the Sun). ...

... 108.1163Kellermann+ J/AJ/108/1163 Radio structure of Quasars (Kellermann+ 1994) ================================================================================ The radio structure of radio loud and radio quiet quasars in the Palomar bright quasar survey. ... The observed structure of some well resolved radio quiet quasars and AGN's show large scale linear structures or unresolved central cores similar to radio loud objects in the BQS sample as well as the more luminous radio selected quasars. ...

... Science . ... Science Users Information > Science and Technical Meetings > Conferences 2002 > cosmology2002 . ... Observing with ESO Telescopes . ... Public Surveys . ... Data Handling and Products . ... Science Data Products Forum . ... ESO Data . ... ESO Data Access Policy . ... Review: Weak Lensing . ... Tangential alignement of galaxies in a STIS Parallel shear survey field: a new dark lens candidate . ... Poster: . ... New Clues on clustering evolution from the K20 and FIRES surveys . ... data ...

Gleb Koshevoy (CEMI RAS and Poncelet lab) and Gerard van der Laan (Free University of Amsterdam) . ... The workshop will start on Monday morning, May 29, and end of Friday afternoon, June 2. The morning is panned for 1 and 1/2 hours talks and the afternoon is reserved for discussions. Morning lectures start at 10:00 and are scheduled at rooms 816 or 520 (CEMI), afternoon discussions are at rooms 816 (CEMI) or 408 (Poncelet lab). ... Poncelet lab is at IMU, Bol'shoi Vlas'evskii, 11 . ...