BeppoSAX Observations of Centaurus A: the Hard Continuum and the Iron Line Feature
| Autor: | Laura Maraschi, Giorgio Matt, E. Massaro, A. Preite-Martinez, C. M. Urry, C. Perola, Werner Collmar, Paola Grandi, Helmut Steinle, Mariateresa Fiocchi |
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| Přispěvatelé: | Grandi, P, Fiocchi, M, Perola, Cg, Urry, Cm, Maraschi, L, Massaro, E, Matt, Giorgio, Preite Martinez, A, Steinle, H, Collmar, W. |
| Jazyk: | angličtina |
| Rok vydání: | 2003 |
| Předmět: | |
| Zdroj: | 593 (2003): 160–168. info:cnr-pdr/source/autori:Grandi, P.; Fiocchi, M.; Perola, C. G.; Urry, C. M.; Maraschi, L.; Massaro, E.; Matt, G.; Preite-Martinez, A.; Steinle, H.; Collmar, W./titolo:BeppoSAX Observations of Centaurus A: The Hard Continuum and the Iron-Line Feature/doi:/rivista:/anno:2003/pagina_da:160/pagina_a:168/intervallo_pagine:160–168/volume:593 |
| Popis: | The radio galaxy Centaurus A was observed by the BeppoSAX satellite five times from 1997 to 2000. From July 6 1999 to August 17 1999, the source was also simultaneously pointed by COMPTEL on-board of the satellite CGRO. Centaurus A has a complex spectrum with multiple extended components and a strongly absorbed (N_H\sim 10^{23}$ cm${-2}) nucleus well fitted by a power law (\Gamma \sim 1.8) which bends at high energies. When the BeppoSAX and COMPTEL observations are combined together, an exponential cutoff with e-folding energy \sim 1000 keV gives an adequate description of the spectral steepening. A complex feature in emission at 6-7 keV is resolved into two Fe components, one narrow cold line and an ionized line centred at 6.8 keV. Significant variations have been observed in the iron feature, with the less prominent ionized line seemingly being the only one responsible for them: its variations do not appear to correlate with the strength of the continuum. The high energy cutoff and the Fe feature suggest the presence of an accretion flow in the Centaurus A nucleus. However the absence of a significant reflection, the narrowness of the cold line as well as the lack of correlation between the continuum and 6.8 keV line variations disfavour a standard cold/ionized thin disk (at least in the inner regions). A more plausible configuration might be a hot thick optically thin accretion flow surrounded by material with different opacities. Finally, we note that high energy break observed by BeppoSAX and COMPTEL could be also reasonably explained by Inverse Compton radiation from a jet. If this is the case, a structured jet with outer slow layers surrounding a beamed inner region is necessary to explain the strong Fe feature observed by BeppoSAX. Comment: 21 pages, 8 figures, accepted for publication in ApJ |
| Databáze: | OpenAIRE |
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