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

作者：Yasumi Masato^*; Nobukawa Masayoshi; Nakashima Shinya; Uchida Hiroyuki; Sugawara Ryusuke; Tsuru Takeshi Go; Tanaka Takaaki; Koyama Katsuji

来源：Publications of the Astronomical Society of Japan, 2014, 66(4): 68.

DOI：10.1093/pasj/psu043

• ISM: supernova remnants
• X-rays: individual (G350.1-0.3, G349.7+0.2)
• X-rays: ISM

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 K alpha 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 non-equilibrium 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 similar to 15-25M(circle dot) for G350.1-0.3 and similar to 35-40M(circle dot) for G349.7+0.2. We find extremely high abundances of Ni compared to Fe (Z(Ni)/Z(Fe) similar to 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 similar to 13M(circle dot) and similar to 24M(circle dot) for G350.1-0.3 and G349.7+0.2, respectively. These values are consistent with the progenitor masses of similar to 15-25M(circle dot) and similar to 35-40M(circle dot) for G350.1-0.3 and G349.7+0.2, respectively.

• 出版日期2014-8