机译:银河系隆起中来自宇宙黎明的极贫金属恒星
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Univ Cambridge, Inst Astron, Cambridge CB3 0HA, England;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Univ Warsaw Observ, PL-00473 Warsaw, Poland|Ohio State Univ, Dept Astron, Columbus, OH 43210 USA;
Uppsala Univ, Div Astron & Space Phys, Dept Phys & Astron, SE-75120 Uppsala, Sweden;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia|Univ Hertfordshire, Sch Phys Astron & Math, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Max Planck Inst Astron, D-69117 Heidelberg, Germany;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia;
Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2601, Australia|Univ Paris 06, Univ Paris 04, F-75014 Paris, France|CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland|Univ Concepcion, Dept Astron, Concepcion, Chile;
Univ Warsaw Observ, PL-00473 Warsaw, Poland|Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
Univ Warsaw Observ, PL-00473 Warsaw, Poland;
机译:银河系中极度贫金属的恒星:电离后形成的第二代
机译:银河系中极度贫金属的恒星:电离后形成的第二代
机译:银河极星中Mg和K的非LTE丰度以及银河系中[O / Mg],[Na / Mg],[Al / Mg]和[K / Mg]的演化
机译:银河系中的极端金属贫瘠的星星
机译:贫金属恒星的元素丰度可以追溯到银河系厚盘的起源
机译:一贫金属星系中的一氧化碳
机译:在银河系隆起的宇宙黎明中,极度金属贫瘠的恒星