Search Results - "Churazov Eugene"

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    Sound wave generation by a spherically symmetric outburst and AGN feedback in galaxy clusters by Tang, Xiaping, Churazov, Eugene

    “…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 by Anderson, Michael E., Churazov, Eugene, Bregman, Joel N.

    “…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 by Zhang, Congyao, Churazov, Eugene, Schekochihin, Alexander A

    “…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 by Di Mascolo, Luca, Churazov, Eugene, Mroczkowski, Tony

    “…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 by Zhang, Congyao, Churazov, Eugene, Forman, William R, Lyskova, Natalia

    “…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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    Progressive steepening of the SNR RX J1713.7–3946 X-ray spectrum from XMM–Newton to INTEGRAL by Kuznetsova, Ekaterina, Krivonos, Roman, Churazov, Eugene, Lyskova, Natalia, Lutovinov, Alexander

    “…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 by Su, Yuanyuan, Kraft, Ralph P., Roediger, Elke, Nulsen, Paul, Forman, William R., Churazov, Eugene, Randall, Scott W., Jones, Christine, Machacek, Marie E.

    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 by Wu, Xufen, Gerhard, Ortwin, Naab, Thorsten, Oser, Ludwig, Martinez-Valpuesta, Inma, Hilz, Michael, Churazov, Eugene, Lyskova, Natalya

    “…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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    The BIG X-ray tail by Ge, Chong, Sun, Ming, Yagi, Masafumi, Fossati, Matteo, Forman, William, Jáchym, Pavel, Churazov, Eugene, Zhuravleva, Irina, Boselli, Alessandro, Jones, Christine, Ji, Li, Luo, Rongxin

    “…ABSTRACT Galaxy clusters grow primarily through the continuous accretion of group-scale haloes. Group galaxies experience preprocessing during their journey…”
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    Hard X-ray emission of Sco X-1 by Revnivtsev, Mikhail G, Tsygankov, Sergey S, Churazov, Eugene M, Krivonos, Roman A

    “…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 by Churazov, Eugene, Zhuravleva, Irina, Sazonov, Sergey, Sunyaev, Rashid

    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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    Probing the structure of the gas in the Milky Way through X-ray high-resolution spectroscopy by Gatuzz, Efraín, Churazov, Eugene

    “…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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