X-ray spectroscopy of the LINER NGC7213

GT Detailed Xray spectral information will help to distinguish between theemission mechanisms present in this bright LINER. If it contains a .dwarf. AGN,it should show a compact, variable source whose Xray emission has a nonthermalpowerlaw form. It may also show strong Fe Kalpha line emission produced byfluorescence in cold matter. On the other hand, nuclear starbursts arefrequently extended over kpc scales and are expected to show thermal spectracharacterised by coronal Xray emission lines. truncated!, Please see actual data for full text [truncated!, Please see actual data for full text]