Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S322(11), p. 208-209, 2016
DOI: 10.1017/s1743921316012059
Full text: Unavailable
AbstractOver the past 15 years, the molecular complex Sgr C has been repeatedly observed with both XMM-Newton and Chandra. These observations reveal new features indicating that the region might be more complex than previously thought. We find that its strong iron line emission at 6.4 keV varies significantly over time, which supports the X-ray reflection scenario.