Predicting the X-ray brightness distributions of cluster sources – I. Estimating the potentials
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/185/3/473/18521205/mnras185-0473.pdf
Cited by 26 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. X-ray shapes of elliptical galaxies and implications for self-interacting dark matter;Journal of Cosmology and Astroparticle Physics;2021-05-01
2. Cosmological simulations with self-interacting dark matter – II. Halo shapes versus observations;Monthly Notices of the Royal Astronomical Society;2013-01-24
3. CONSTRAINING CLUSTER PHYSICS WITH THE SHAPE OF X-RAY CLUSTERS: COMPARISON OF LOCAL X-RAY CLUSTERS VERSUS ΛCDM CLUSTERS;The Astrophysical Journal;2012-08-02
4. Spherically averaging ellipsoidal galaxy clusters in X-ray and Sunyaev-Zel’dovich studies - II. Biases;Monthly Notices of the Royal Astronomical Society;2012-01-19
5. Dark Matter in Elliptical Galaxies;Hot Interstellar Matter in Elliptical Galaxies;2011-08-09
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