Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S322(11), p. 208-209, 2016

DOI: 10.1017/s1743921316012059

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An X-ray view of Sagittarius C

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

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Data provided by SHERPA/RoMEO

Abstract

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.

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