Cold gas in the intracluster medium: implications for flow dynamics and powering optical nebulae
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/389/3/1259/3334042/mnras0389-1259.pdf
Reference32 articles.
1. A Systematic Study of Radio‐induced X‐Ray Cavities in Clusters, Groups, and Galaxies
2. Heat conduction boundary layers of condensed clumps in cooling flows
3. The ROSAT Brightest Cluster Sample -- III. Optical spectra of the central cluster galaxies
4. Emission-line nebulae around central cluster galaxies in cooling flows
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1. TURBULENT MOLECULAR GAS AND STAR FORMATION IN THE SHOCKED INTERGALACTIC MEDIUM OF STEPHAN'S QUINTET;The Astrophysical Journal;2012-04-04
2. A MOLECULAR HYDROGEN NEBULA IN THE CENTRAL cD GALAXY OF THE PERSEUS CLUSTER;The Astrophysical Journal;2011-12-20
3. First observations of CN (2-1), HCO+ (3-2) and C2H (3-2) emission lines in the Perseus cluster: constraints on heating mechanisms in the cluster gas;Monthly Notices of the Royal Astronomical Society;2011-09-07
4. Molecular tracers of filamentary CO emission regions surrounding the central galaxies of clusters;Astronomy and Astrophysics;2010-10
5. ON THE ORIGIN OF THE EXTENDED Hα FILAMENTS IN COOLING FLOW CLUSTERS;The Astrophysical Journal;2010-09-08
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