Kavli Affiliate: Shinichiro Takeda | Summary:Thanks to its high spectral resolution (~5 eV at 6 keV), the Soft X-ray Spectrometer (SXS) on board Hitomi enables us to measure the detailed structure of spatially resolved emission lines from highly ionized ions in galaxy clusters for the first time. In this series of papers, using the SXS […]
Continue.. Measurements of resonant scattering in the Perseus cluster core with Hitomi SXS