Department of Earth and Space Science, Graduate School of Science,Osaka University, 1-1 Machikaneyama-machi, Toyonaka, Osaka, 560-0043;
Department of Physics, Graduate School of Science, Kyoto University,Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-8502;
Department of Physics, Graduate School of Science, Kyoto University,Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-8502;
Department of Physics, Graduate School of Science, Kyoto University,Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-8502;
Department of Physics, Graduate School of Science, Kyoto University,Kitashirakawa Oiwake-cho, Sakyo-ku, Kyoto, 606-8502;
et al;
Galaxy; center — ISM; clouds — ISM; molecules — X-rays; ISM;
机译:人马座C区中性铁K $ alpha $线等效宽度大的X射线反射星云
机译:Sgr B1地区的X射线反射星云和新的超新星残留候选者的朱雀光谱。
机译:Sgr B1区X射线反射星云和新的超新星残留候选者的朱雀光谱
机译:SGR C地区的中性铁k-alpha线具有大量等效宽度的X射线反射星云
机译:X射线反射的铁K-α发射:γ射线的预测 爆裂模型
机译:seyfert 2 Galaxy NGC 2110:Nustar观察到的硬X射线发射和铁K-alpha线的变异性。