XRISM collaboration’s first paper on the LMC supernova remnant N132D has been accepted for publication in PASJ (ADS link). We successfully constrained the line widths and redshifts, and thereby confidently separated multiple temperature components. The narrow lines of Si, S, and Ar, and a broad Fe Hea triplet can be understood as due to different ion temperatures. Discussion based on line broadening is so exciting as it is brand new in the field of supernova remnants.
XRISM first paper on supernova remnant N132D!
Astrophysical Research Works of Hiromasa Suzuki 