. english || русский . Main . Location . Telescope . Instruments . Program . Science . Publications . Images . Photos . Links . Observations of galaxy clusters from 400 square degree cluster survey. Optical identifications of new INTEGRAL, SWIFT and RXTE hard X-ray sources. Fast optical photometry of SS433. Observations of gamma-ray bursts optical afterglows. High Energy Astrophysics Department 2016 IKI RAN

Lack of co oling flow clusters at z 0.5 A. Vikhlinin1,2 , R. Burenin2 , W. R. Forman1 , C. Jones1 , A. Hornstrup3 , S. S. Murray1, and H. Quintana4 1 2 3 4 Harvard-Smithsonian ... Astronomia y Astrofisica, Pontificia Universidad Catolica de Chile The goal of this work is to study the incidence rate of co oling flows in the high redshift clusters using Chandra observations of z 0.5 ob jects from a new large, ... Fig. ... Lack of "cooling flow" clusters at z > 0.5 3 Fig. ...