Limits on turbulent propagation of energy in cool-core clusters of galaxies-Reference-Cited by-同舟云学术

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Limits on turbulent propagation of energy in cool-core clusters of galaxies

Published:2018-04-17 Issue:1 Volume:478 Page:L44-L48
ISSN:1745-3925
Container-title:Monthly Notices of the Royal Astronomical Society: Letters
language:en
Short-container-title:

Author:

Bambic C J¹²^ORCID,Pinto C²^ORCID,Fabian A C²,Sanders J³^ORCID,Reynolds C S¹²^ORCID

Affiliation:

1. Department of Astronomy, University of Maryland, College Park, MD 20742-2421, USA

2. Institute of Astronomy, Madingley Road, CB3 0HA Cambridge, UK

3. Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse 1, D-85748 Garching, Germany

Funder

European Research Council

National Sleep Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnrasl/article-pdf/478/1/L44/25027045/sly060.pdf

Reference26 articles.

1. Resonant excitation of internal gravity waves in cluster cooling flows

2. AGN jet feedback on a moving mesh: cocoon inflation, gas flows and turbulence

3. Estimating turbulent velocities in the elliptical galaxies NGC 5044 and NGC 5813

4. Investigating AGN heating in a sample of nearby clusters

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1. Gas rotation and dark matter halo shape in cool-core clusters of galaxies;Astronomy & Astrophysics;2024-01-31

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3. Radio jet–ISM interaction and positive radio-mechanical feedback in Abell 1795;Monthly Notices of the Royal Astronomical Society;2022-12-29

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

5. The cycle of metals in the infalling elliptical galaxy NGC 1404;Monthly Notices of the Royal Astronomical Society;2022-01-29

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