X‐Ray Observations of the Coma Cluster in a Broad Energy Band with theINTEGRAL,RXTE, andROSATObservatories-Reference-Cited by-同舟云学术

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X‐Ray Observations of the Coma Cluster in a Broad Energy Band with theINTEGRAL,RXTE, andROSATObservatories

Published:2008-11-10 Issue:2 Volume:687 Page:968-975
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:Astrophysical Journal

Author:

Lutovinov A. A.,Vikhlinin A.,Churazov E. M.,Revnivtsev M. G.,Sunyaev R. A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference40 articles.

1. XMM-Newton observation of the Coma Galaxy cluster

2. Particle reacceleration in the Coma cluster: radio properties and hard X-ray emission

3. Where does the hard X-ray diffuse emission in clusters of galaxies come from?

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1. Discovery of inverse-Compton X-ray emission and estimate of the volume-averaged magnetic field in a galaxy group;MON NOT R ASTRON SOC;2023

2. Baryon cycles in the biggest galaxies;Physics Reports;2022-08

3. Progressive steepening of the SNR RX J1713.7–3946 X-ray spectrum from XMM–Newton to INTEGRAL;Monthly Notices of the Royal Astronomical Society;2019-08-16

4. INTEGRAL/IBIS deep extragalactic survey: M81, LMC and 3C 273/Coma fields;Monthly Notices of the Royal Astronomical Society;2016-03-15

5. COSMIC RAYS IN GALAXY CLUSTERS AND THEIR NONTHERMAL EMISSION;International Journal of Modern Physics D;2014-03-18

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