{ "id": "astro-ph/9808042", "version": "v1", "published": "1998-08-05T20:48:44.000Z", "updated": "1998-08-05T20:48:44.000Z", "title": "Observation of Cen A by the Rossi X-ray Timing Explorer", "authors": [ "R. E. Rothschild", "D. L. Band", "P. R. Blanco", "D. E. Gruber", "W. A. Heindl", "D. R. MacDonald", "D. C. Marsden", "K. Jahoda", "D. Pierce", "G. Madejski", "M. Elvis", "D. A. Schwartz", "R. Remillard", "A. A. Zdziarski", "C. Done", "R. Svensson" ], "comment": "24 pages, 3 figures, accepted to The Astrophysical Journal", "doi": "10.1086/306618", "categories": [ "astro-ph" ], "abstract": "The Rossi X-ray Timing Explorer made a short (10 ks) observation of the radio galaxy Centaurus A on 14 August 1996. Analysis of the combined 2.5-240 keV spectrum has revealed a heavily absorbed(NH=9.42+/-0.24 e22 cm-2) primary power law (index=1.86+/-0.015) and an iron line due to fluorescence of cold matter (EW=162+/-25 eV). Flux from either a jet, primary flux scattered into the line of sight, or primary flux seen through a partial absorber was not required. The iron line width is unresolved at the 95% confidence level (sigma < 0.54 keV). No significant variability in the iron line flux is seen from measurements over the last two decades, while the overall continuum flux varied by more than a factor of four, which implies that the line emission region is distant from that of the primary emission. While radio-quiet Seyfert galaxies exhibit spectral components attributable to Compton reflection from cold matter, Cen A reveals no such component (exposed solid angle ratio < 0.09). This supports unified models of active galaxies that have little difference between Seyfert 2 and low luminosity radio galaxies", "revisions": [ { "version": "v1", "updated": "1998-08-05T20:48:44.000Z" } ], "analyses": { "keywords": [ "rossi x-ray timing explorer", "radio galaxy", "iron line", "observation", "low luminosity radio galaxies" ], "tags": [ "journal article" ], "note": { "typesetting": "TeX", "pages": 24, "language": "en", "license": "arXiv", "status": "editable", "inspire": 489855 } } }