Fe K line complex in the nuclear region of NGC 253
  A bright, nearby edge-on starburst galaxy NGC 253 was studied using the
Suzaku, XMM and Chandra X-ray observatories. We detected with Suzaku and XMM
complex line structure of Fe K, which is resolved into three lines (Fe I at 6.4
keV, Fe XXV at 6.7 keV and Fe XXVI at 7.0 keV) around the center of NGC 253.
Especially, the Fe I and Fe XXVI lines are the first clear detections, with a
significance of >99.99 % and 99.89 % estimated by a Monte Carlo procedure.
Imaging spectroscopy with Chandra revealed that the emission is distributed in
~60 arcsec^2 region around the nucleus, which suggests that the source is not
only the buried AGN. The flux of highly ionized Fe lines can be explained by
the accumulation of 10-1000 supernova remnants that are the result of high
starforming activity, while the Fe I line flux is consistent with the
fluorescent line emission expected with the molecular clouds in the region.
