Molecular accretion in the core of the galaxy cluster 2A 0335+096
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/416/3/2060/2851188/mnras0416-2060.pdf
Reference43 articles.
1. The relation between accretion rate and jet power in X-ray luminous elliptical galaxies
2. An Entropy Threshold for Strong Hα and Radio Emission in the Cores of Galaxy Clusters
3. The ROSAT Brightest Cluster Sample -- III. Optical spectra of the central cluster galaxies
4. The Star‐forming Torus and Stellar Dynamical Black Hole Mass in the Seyfert 1 Nucleus of NGC 3227
5. Star Formation, Radio Sources, Cooling X-Ray Gas, and Galaxy Interactions in the Brightest Cluster Galaxy in 2A0335+096
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1. The jet feedback mechanism (JFM) in stars, galaxies and clusters;New Astronomy Reviews;2016-12
2. MOLECULAR GAS ALONG A BRIGHT HαFILAMENT IN 2A 0335+096 REVEALED BY ALMA;The Astrophysical Journal;2016-11-29
3. Rescuing the intracluster medium of NGC 5813;Research in Astronomy and Astrophysics;2016-06
4. Optical emission line nebulae in galaxy cluster cores 1: the morphological, kinematic and spectral properties of the sample;Monthly Notices of the Royal Astronomical Society;2016-05-06
5. Heating the intracluster medium by jet-inflated bubbles;Monthly Notices of the Royal Astronomical Society;2015-11-19
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