Evidence for a clumpy disc-wind in the star forming Seyfert\,2 galaxy MCG--03--58--007
| Autor: | Matzeu, G. A., Braito, V., Reeves, J. N., Severgnini, P., Ballo, L., Caccianiga, A., Campana, S., Cicone, C., Della Ceca, R., Parker, M. L., Santos-Lleó, M., Schartel, N. |
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| Rok vydání: | 2018 |
| Předmět: | |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1093/mnras/sty3327 |
| Popis: | We report the results of a detailed analysis of a deep simultaneous $130\,\rm ks$ \textit{XMM-Newton & NuSTAR} observation of the nearby ($z=0.0315$) and bright ($L_{\rm bol}\sim3\times10^{45}\,\rm erg\,s^{-1}$) starburst-AGN Seyfert\,2 system: MCG--03--58--007. From the broadband fitting we show that most of the obscuration needs to be modeled with a toroidal type reprocessor such as \texttt{MYTorus} \citep{MurphyYaqoob09}. Nonetheless the signature of a powerful disc-wind is still apparent at higher energies and the observed rapid short-term X-ray spectral variability is more likely caused by a variable zone of highly ionized fast wind rather than by a neutral clumpy medium. We also detect X-ray emission from larger scale gas as seen from the presence of several soft narrow emission lines in the RGS, originating from a contribution of a weak star forming activity together with a dominant photoionized component from the AGN. Comment: 16 pages, 9 figures, accepted for publication in MNRAS |
| Databáze: | arXiv |
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