Abundances in the ejecta of core-collapse supernova remnants G350.1-0.3 and G349.7+0.2

Abstract

We present Suzaku results of the two Galactic supernova remnants (SNRs) G350.1-0.3 and G349.7+0.2. We find Al and Ni Kα lines from both the SNRs for the first time, in addition to previously detected K-shell lines of Mg, Si, S, Ar, Ca, and Fe. The spectra are well described by two optically thin thermal plasmas: a low-temperature (low-kT) plasma in collisional ionization equilibrium and a high-temperature (high-kT) plasma in nonequilibrium ionization. Since the low-kT plasma has solarmetal abundances, it is thought to be of interstellar medium origin. The high-kT plasma has super-solar abundances, hence it is likely to be of ejecta origin. The abundance patterns of the ejecta components are similar to those of core-collapse supernovae with progenitor masses of ~15-25M⊙ for G350.1-0.3 and ~35-40M⊙ for G349.7+0.2. We find extremely high abundances of Ni compared to Fe (Z Ni/ZFe ~ 8). Based on the measured column densities between the SNRs and the near sky background, we propose that G350.1-0.3 and G349.7+0.2 are located at distances of 9±3kpc and 12±5 kpc, respectively. Then the ejecta masses are estimated to be ~13M⊙ and ~24M⊙ for G350.1-0.3 and G349.7+0.2, respectively. These values are consistent with the progenitor masses of ~15-25M⊙ and ~35-40M⊙ for G350.1-0.3 and G349.7+0.2, respectively. © The Author 2014.