Found: 22
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Metal enrichment: The apex accretor perspective.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202346918
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- Article
CHEX-MATE: Characterization of the intra-cluster medium temperature distribution.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 682, p. 1, doi. 10.1051/0004-6361/202346651
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- Article
The Planck clusters in the LOFAR sky: IV. LoTSS-DR2: Statistics of radio haloes and re-acceleration models.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 672, p. 1, doi. 10.1051/0004-6361/202244876
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- Article
CHEX-MATE: Pressure profiles of six galaxy clusters as seen by SPT and Planck.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 672, p. 1, doi. 10.1051/0004-6361/202245012
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The Planck clusters in the LOFAR sky: III. LoTSS-DR2: Dynamic states and density fluctuations of the intracluster medium.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 672, p. 1, doi. 10.1051/0004-6361/202244761
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- Article
PHEMTO: the polarimetric high energy modular telescope observatory.
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- Experimental Astronomy, 2021, v. 51, n. 3, p. 1143, doi. 10.1007/s10686-021-09723-x
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- Article
The XXL Survey: XLII. Detection and characterisation of the galaxy population of distant galaxy clusters in the XXL-N/VIDEO field: A tale of variety.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038982
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Non-thermal pressure support in X-COP galaxy clusters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 621, p. N.PAG, doi. 10.1051/0004-6361/201833324
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Hydrostatic mass profiles in X-COP galaxy clusters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 621, p. N.PAG, doi. 10.1051/0004-6361/201833323
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The XMM Cluster Outskirts Project (X-COP): Thermodynamic properties of the intracluster medium out to R200 in Abell 2319.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2018, v. 614, p. N.PAG, doi. 10.1051/0004-6361/201731748
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- Article
A systematic analysis of the XMM-Newton background: IV.
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- Experimental Astronomy, 2017, v. 44, n. 3, p. 321, doi. 10.1007/s10686-017-9549-y
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Deep Chandra observations of the stripped galaxy group falling into Abell 2142.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2017, v. 605, p. 1, doi. 10.1051/0004-6361/201730555
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- Article
The XXL survey: First results and future.
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- Astronomische Nachrichten, 2017, v. 338, n. 2/3, p. 334, doi. 10.1002/asna.201713352
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XIII. Baryon content of the bright cluster sample.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2016, v. 592, p. 1, doi. 10.1051/0004-6361/201527293
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XII. Optical spectroscopy of X-ray-selected clusters and the frequency of AGN in superclusters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2016, v. 592, p. 1, doi. 10.1051/0004-6361/201526976
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VII. A supercluster of galaxies at z = 0.43.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2016, v. 592, p. 1, doi. 10.1051/0004-6361/201527142
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The evolution of the spatially resolved metal abundance in galaxy clusters up to z = 1.4 (Research Note).
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2015, v. 578, p. 1, doi. 10.1051/0004-6361/201425470
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The stripping of a galaxy group diving into the massive cluster A2142.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2014, v. 570, p. 1, doi. 10.1051/0004-6361/201424259
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A phase-variable absorption feature in the X-ray spectrum of the magnetar SGR 0418+5729.
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- Astronomische Nachrichten, 2014, v. 335, n. 3, p. 274, doi. 10.1002/asna.201312031
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Abell 2142 at large scales: An extreme case for sloshing?
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2013, v. 556, n. 6, p. 1, doi. 10.1051/0004-6361/201321319
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- Article
The gas distribution in the outer regions of galaxy clusters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 541, p. 1, doi. 10.1051/0004-6361/201118281
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An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2012, v. 537, p. 1, doi. 10.1051/0004-6361/201117836
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