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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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Proceedings ArticleDOI

The large observatory for x-ray timing

Marco Feroci, +343 more
- 31 Jul 2014 - 
TL;DR: The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final downselection for a launch slot in 2022-2024 as mentioned in this paper.
Journal ArticleDOI

Cyclo-synchrotron emission from magnetically dominated active regions above accretion discs

TL;DR: In this paper, the role of thermal cyclo-synchrotron emission in a magnetically dominated corona above an accretion disk in an active galaxy or a galactic black hole candidate is discussed.
Journal ArticleDOI

A tale of two periods: determination of the orbital ephemeris of the super-Eddington pulsar NGC 7793 P13

TL;DR: In this paper, the authors present a timing analysis of multiple XMM-Newton and NuSTAR observations of the ultra-luminous pulsar NGC 7793 P13 spread over its 65d variability period.
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The X-ray subcluster in A 2256: cluster mergers, cooling flows and diffuse radio sources

TL;DR: In this paper, the fate of the gas in a merging subcluster is discussed and it is shown that it may not be shocked during the merger, if either cluster or sub-cluster contains a cooling flow the cooling gas will not necessarily be reheated but can thermalize its bulk kinetic energy in the less dense hot gas.
Journal ArticleDOI

The relation between line emission and brightest cluster galaxies in three exceptional clusters : evidence for gas cooling from the intracluster medium.

TL;DR: In this paper, the authors combine integral field spectroscopy, CO observations and X-ray data to study three exceptional clusters (Abell 1991, Abell 3444 and Ophiuchus) where there is a physical and dynamical offset between the BCG and the cooling peak to investigate the connection between the cooling of the ICM, the cold gas being deposited and the central galaxy.