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A. C. Fabian
Researcher at University of Cambridge
Publications - 820
Citations - 43942
A. C. Fabian is an academic researcher from University of Cambridge. The author has contributed to research in topics: Galaxy & Active galactic nucleus. The author has an hindex of 103, co-authored 818 publications receiving 41589 citations.
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Journal ArticleDOI
Detection of optical coronal emission from 106-K gas in the core of the Centaurus cluster
R. E. A. Canning,A. C. Fabian,R. M. Johnstone,Jeremy S. Sanders,C. S. Crawford,Nina A. Hatch,Gary J. Ferland +6 more
TL;DR: In this article, a detection of the optical coronal emission line [Fe X]�6374 and upper limits of four other coronal lines using high resolution VIMOS spectra centred on NGC 4696, the brightest cluster galaxy in the Centaurus cluster was reported.
Journal ArticleDOI
Soft X-ray background fluctuations and large-scale structure in the Universe
TL;DR: In this paper, the authors studied the fluctuations of the soft (0.9-2 keV) X-ray background in the presence of confusion noise produced by sources unresolved with the beam sizes.
Journal ArticleDOI
Fe emission and ionized excess absorption in the luminous quasar 3C 109 with XMM–Newton
TL;DR: In this article, the authors reported results from an XMM-Newton observation of the broad-line radio galaxy 3C 109 (z=0.3056), which revealed the presence of a broad iron line from the accretion disc with which the X-ray spectrum is fully consistent.
Journal ArticleDOI
Detection of optical coronal emission from 10^6 K gas in the core of the Centaurus cluster
Rebecca E. A. Canning,A. C. Fabian,R. M. Johnstone,Jeremy S. Sanders,C. S. Crawford,Nina A. Hatch,Gary J. Ferland +6 more
TL;DR: In this paper, a detection of the optical coronal emission line [Fe X]6374 and upper limits of four other coronal lines using high resolution VIMOS spectra centred on NGC 4696, the brightest cluster galaxy in the Centaurus cluster.
Journal ArticleDOI
Continuing formation of the central star cluster in M87
TL;DR: In this article, the authors show that the back-reaction on the flow of the nuclear luminosity is small unless M87 was much brighter in the past and suggest that massive central star clusters may be common in the central galaxies in many clusters and, on a smaller scale, in many elliptical galaxies.