Recombining Plasma and Hard X-Ray Filament in the Mixed-Morphology Supernova Remnant W 44
Yamaguchi, Hiroya; Uchida, Hiroyuki; Fukui, Yasuo; Tsuru, Takeshi Go; Tanaka, Takaaki; Sawada, Makoto; Ohnishi, Takao; Yoshiike, Satoshi; Katsuji, Koyama
Japan, United States
Abstract
We report on new features of the typical mixed-morphology supernova remnant W 44. In X-ray spectra obtained with Suzaku, radiative recombination continua of highly ionized atoms were detected for the first time. The spectra are well reproduced by a thermal plasma in a recombining phase. The best-fit parameters suggest that the electron temperature of the shock-heated matter rapidly cooled down from $\sim$ 1 keV to $\sim$ 0.5 keV, possibly due to adiabatic expansion (rarefaction), occurred $\sim$ 20000 yr ago. We also discovered hard X-ray emission, which shows an arclike structure spatially correlating with a radio continuum filament. The surface-brightness distribution has a clear anticorrelation with $^{12}$ CO ($J$ $=$ 2-1) emission from a molecular cloud observed with NANTEN2. While the hard X-ray is most likely due to a synchrotron enhancement in the vicinity of the cloud, no current model can quantitatively predict the observed flux.