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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
A Comparison of Intermediate-Mass Black Hole Candidate Ultraluminous X-Ray Sources and Stellar-Mass Black Holes
TL;DR: In this article, the authors compare the inferred disk temperatures and luminosities of a small number of ultraluminous X-ray sources (ULXs) with LX ≥ 1040 ergs s-1 in nearby galaxies.
Journal ArticleDOI
EXOSAT observations of a strong soft X-ray excess in MKN 841.
Keith A. Arnaud,Graziella Branduardi-Raymont,J. L. Culhane,A. C. Fabian,C. Hazard,C. Hazard,T. A. McGlynn,T. A. McGlynn,R. A. Shafer,A. F. Tennant,Martin Ward +10 more
TL;DR: Les observations EXOSAT du spectre de Mkn 841 montrent qu'il est bien represente par une loi de puissance d'indice 1,6, semblable a celui des autres Seyfert, a laquelle s'ajoute une grande composante additionnelle as mentioned in this paper.
Journal ArticleDOI
A Comparison of Intermediate Mass Black Hole Candidate ULXs and Stellar-Mass Black Holes
TL;DR: In this paper, the authors compare the inferred disk temperatures and luminosities of a small number of ultra-luminous X-ray (ULX) sources with L_X > 1 E+40 erg/s in nearby galaxies.
Journal ArticleDOI
Properties of cooling flows in a flux-limited sample of clusters of galaxies
TL;DR: In this article, the mass flow rates of cooling flows in an X-ray flux-limited sample of clusters of galaxies, in which most of the clusters have been observed with both imaging and spectroscopic detectors, are presented.
Journal ArticleDOI
Revealing the Dusty Warm Absorber in MCG--6-30-15 with the Chandra HETG
Julia C. Lee,P. M. Ogle,Claude R. Canizares,H. L. Marshall,Norbert S. Schulz,R. Morales,A. C. Fabian,K. Iwasawa +7 more
TL;DR: In this article, the authors present detailed evidence for a warm absorber in the Seyfert 1 galaxy MCG and dispute earlier claims for relativistic O line emission.