机译:在银河系中的低质量恒星之前红色巨型阶段的巨大锂增强?
Key Lab of Optical Astronomy National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 People?s Republic of China;
National Astronomical Observatory of Japan Mitaka Tokyo 181-8588 Japan;
National Astronomical Observatory of Japan Mitaka Tokyo 181-8588 Japan;
Key Lab of Optical Astronomy National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 People?s Republic of China;
Key Lab of Optical Astronomy National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 People?s Republic of China;
Research Center for the Early Universe Graduate School of Science University of Tokyo Hongo Tokyo 113-0033 Japan;
Key Lab of Optical Astronomy National Astronomical Observatories Chinese Academy of Sciences Beijing 100012 People?s Republic of China;
nuclear reactions; nucleosynthesis; abundances; stars: abundances; stars: evolution; stars: low-mass; stars: Population II;
机译:在银河系中的低质量恒星之前红色巨型阶段的巨大锂增强?
机译:低质量红色巨星中氦气中的氦核心质量:观测和理论
机译:晕(现金)项目中恒星的遥远的望远镜化学丰度。 I.锂,s和r增强的贫金属巨型HKII 17435-00532
机译:非常低质量的星星,银河系中的金属极低金属
机译:使用SDSS-II SN调查RR天琴座星系探索银河系光环
机译:向低质量原恒星揭开磁化射流的面纱
机译:中国低质量恒星中红巨星相位前的巨大李增强 银河系的光环