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Turbulent heating in galaxy clusters brightest in X-rays.

• Authors : Zhuravleva I; 1] Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, 452 Lomita Mall, Stanford, California 94305-4085, USA [2] Department of Physics, Stanford University, 382 Via Pueblo Mall, Stanford, California 94305-4060, USA.; Churazov E

• Source: Nature [Nature] 2014 Nov 06; Vol. 515 (7525), pp. 85-7. Date of Electronic Publication: 2014 Oct 26.Publisher: Nature Publishing Group Country of Publication: England NLM ID: 0410462 Publication Model: Print-Electronic Cited

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Self-similar energetics in large clusters of galaxies.

• Authors : Miniati, Francesco; Beresnyak, Andrey

Subjects: GALAXY clusters; GRAVITATIONAL energy; GRAVITATIONAL instability

• Source: Nature; 7/2/2015, Vol. 523 Issue 7558, p59-62, 4p, 3 Diagrams, 2 Graphs

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Stellar mergers as the origin of magnetic massive stars.

• Authors : Schneider, Fabian R. N.; Ohlmann, Sebastian T.; Podsiadlowski, Philipp

• Source: Nature; 10/10/2019, Vol. 574 Issue 7777, p211-214, 4p, 1 Color Photograph, 1 Diagram, 6 Graphs

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Collapsars as a major source of r-process elements.

• Authors : Siegel, Daniel M.; Barnes, Jennifer; Metzger, Brian D.

• Source: Nature; 5/9/2019, Vol. 569 Issue 7755, p241-244, 4p, 2 Color Photographs, 2 Diagrams, 9 Graphs

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The quiescent intracluster medium in the core of the Perseus cluster.

• Source: Nature; 7/7/2016, Vol. 535 Issue 7610, p117-121, 5p, 3 Color Photographs, 7 Graphs

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