Search Results - "Churazov Eugene"
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Sound wave generation by a spherically symmetric outburst and AGN feedback in galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-07-2017)“…Abstract We consider the evolution of an outburst in a uniform medium under spherical symmetry, having in mind active galactic nucleus feedback in the…”
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Non-detection of X-ray emission from sterile neutrinos in stacked galaxy spectra
Published in Monthly notices of the Royal Astronomical Society (01-10-2015)“…We conduct a comprehensive search for X-ray emission lines from sterile neutrino dark matter, motivated by recent claims of unidentified emission lines in the…”
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Generation of internal waves by buoyant bubbles in galaxy clusters and heating of intracluster medium
Published in Monthly notices of the Royal Astronomical Society (21-08-2018)“…ABSTRACT Buoyant bubbles of relativistic plasma in cluster cores plausibly play a key role in conveying the energy from a supermassive black hole to the…”
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A joint ALMA–Bolocam–Planck SZ study of the pressure distribution in RX J1347.5−1145
Published in Monthly notices of the Royal Astronomical Society (11-08-2019)“…ABSTRACT We report the joint analysis of single-dish and interferometric observations of the Sunyaev–Zeldovich (SZ) effect from the galaxy cluster…”
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Runaway merger shocks in galaxy cluster outskirts and radio relics
Published in Monthly notices of the Royal Astronomical Society (01-10-2019)“…ABSTRACT Moderately strong shocks arise naturally when two subclusters merge. For instance, when a smaller subcluster falls into the gravitational potential of…”
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Standoff distance of bow shocks in galaxy clusters as proxy for Mach number
Published in Monthly notices of the Royal Astronomical Society (01-01-2019)Get full text
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Progressive steepening of the SNR RX J1713.7–3946 X-ray spectrum from XMM–Newton to INTEGRAL
Published in Monthly notices of the Royal Astronomical Society (21-10-2019)“…ABSTRACT In this work, we present the first detailed analysis of the supernova remnant RX J1713.7–3946 in the hard X-ray energy range with the Imager on Board…”
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DEEP CHANDRA OBSERVATIONS OF NGC 1404: CLUSTER PLASMA PHYSICS REVEALED BY AN INFALLING EARLY-TYPE GALAXY
Published in The Astrophysical journal (01-01-2017)“…ABSTRACT The intracluster medium (ICM), as a magnetized and highly ionized fluid, provides an ideal laboratory to study plasma physics under extreme conditions…”
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The mass and angular momentum distribution of simulated massive early-type galaxies to large radii
Published in Monthly notices of the Royal Astronomical Society (01-03-2014)“…We study the dark and luminous mass distributions, circular velocity curves (CVCs), line-of-sight kinematics and angular momenta for a sample of 42…”
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A New Class of X-Ray Tails of Early-type Galaxies and Subclusters in Galaxy Clusters: Slingshot Tails versus Ram Pressure Stripped Tails
Published in The Astrophysical journal (01-04-2019)“…We show that there is a new class of gas tails-slingshot tails-that form as a subhalo (i.e., a subcluster or early-type cluster galaxy) moves away from the…”
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The BIG X-ray tail
Published in Monthly notices of the Royal Astronomical Society. Letters (01-11-2021)“…ABSTRACT Galaxy clusters grow primarily through the continuous accretion of group-scale haloes. Group galaxies experience preprocessing during their journey…”
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Circumgalactic Medium on the Largest Scales: Detecting X-Ray Absorption Lines with Large-area Microcalorimeters
Published in The Astrophysical journal (01-08-2023)“…Abstract The circumgalactic medium (CGM) plays a crucial role in galaxy evolution as it fuels star formation, retains metals ejected from the galaxies, and…”
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Developed turbulence and nonlinear amplification of magnetic fields in laboratory and astrophysical plasmas
Published in Proceedings of the National Academy of Sciences - PNAS (07-07-2015)“…The visible matter in the universe is turbulent and magnetized. Turbulence in galaxy clusters is produced by mergers and by jets of the central galaxies and…”
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Hard X-ray emission of Sco X-1
Published in Monthly notices of the Royal Astronomical Society (01-12-2014)“…We study hard X-ray emission of the brightest accreting neutron star Sco X-1 with INTEGRAL observatory. Up to now INTEGRAL have collected ~4 Ms of deadtime…”
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Resonant Scattering of X-ray Emission Lines in the Hot Intergalactic Medium
Published in Space science reviews (01-12-2010)“…While very often a hot intergalactic medium (IGM) is optically thin to continuum radiation, the optical depth in resonant lines can be of order unity or…”
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A polarized view of the hot and violent universe
Published in Experimental astronomy (01-06-2021)“…X-ray polarimetry has long been considered the ‘holy grail’ of X-ray astronomy. Fortunately, after a silence of more than 40 years, the field is now…”
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EXPLORING THE UNUSUALLY HIGH BLACK-HOLE-TO-BULGE MASS RATIOS IN NGC 4342 AND NGC 4291: THE ASYNCHRONOUS GROWTH OF BULGES AND BLACK HOLES
Published in The Astrophysical journal (10-07-2012)“…We study two nearby early-type galaxies, NGC 4342 and NGC 4291, that host unusually massive black holes relative to their low stellar mass. The observed…”
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A space mission to map the entire observable universe using the CMB as a backlight
Published in Experimental astronomy (01-01-2021)“…This Science White Paper, prepared in response to the ESA Voyage 2050 call for long-term mission planning, aims to describe the various science possibilities…”
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Probing the structure of the gas in the Milky Way through X-ray high-resolution spectroscopy
Published in Monthly notices of the Royal Astronomical Society (01-02-2018)“…Abstract We have developed a new X-ray absorption model, called IONeq, which computes the optical depth τ(E) simultaneously for ions of all abundant elements,…”
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