Matzeu, G. A.G. A.MatzeuBRAITO, ValentinaValentinaBRAITOReeves, J. N.J. N.ReevesSEVERGNINI, PaolaPaolaSEVERGNINIBallo, L.L.BalloCACCIANIGA, AlessandroAlessandroCACCIANIGACAMPANA, SergioSergioCAMPANACicone, C.C.CiconeDELLA CECA, RobertoRobertoDELLA CECAParker, M. L.M. L.ParkerSantos-Lleó, M.M.Santos-LleóSchartel, N.N.Schartel2020-12-292020-12-2920190035-8711http://hdl.handle.net/20.500.12386/29309We report the results of a detailed analysis of a deep simultaneous 130 ksXMM-Newton and NuSTAR observation of the nearby (z = 0.0315) and bright (L_bol∼ 3× 10^{45} erg s^{-1}) starburst-active galactic nucleus (AGN) Seyfert 2 system: MCG-03-58-007. From the broad-band fitting we show that most of the obscuration needs to be modelled with a toroidal type reprocessor such as MYTorus. None the less 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 AGNs.STAMPAenArticle10.1093/mnras/sty33272-s2.0-85066992839000462258200106https://academic.oup.com/mnras/article/483/2/2836/52342492019MNRAS.483.2836MFIS/05 - ASTRONOMIA E ASTROFISICA