Detection of optical coronal emission from 106-K gas in the core of the Centaurus cluster

Author:

Canning R. E. A.,Fabian A. C.,Johnstone R. M.,Sanders J. S.,Crawford C. S.,Hatch N. A.,Ferland G. J.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 9 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. Constraining Gas Motions in the Intra-Cluster Medium;Space Science Reviews;2019-02-19

2. Searching for FUV line emission from 107 K gas in massive elliptical galaxies and galaxy clusters as a tracer of turbulent velocities;Monthly Notices of the Royal Astronomical Society;2016-04-12

3. A very deepChandraview of metals, sloshing and feedback in the Centaurus cluster of galaxies;Monthly Notices of the Royal Astronomical Society;2016-01-24

4. A volume-limited sample of X-ray galaxy groups and clusters – III. Central abundance drops;Monthly Notices of the Royal Astronomical Society;2014-12-16

5. Implications of coronal line emission in NGC 4696*;Monthly Notices of the Royal Astronomical Society;2014-11-19

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