机译:Nugrid Stellar数据集。 I.恒星从H到BI的恒星,金属Z = 0.02和Z = 0.01
Univ Hull Dept Math &
Phys EA Milne Ctr Astrophys Kingston Upon Hull HU6 7RX N Humberside England;
Univ Victoria Dept Phys &
Astron Victoria BC V8P 5C2 Canada;
Keele Univ Keele ST5 5BG Staffs England;
Keele Univ Keele ST5 5BG Staffs England;
LANL Computat Phys &
Methods CCS 2 Los Alamos NM 87545 USA;
LANL Computat Phys &
Methods CCS 2 Los Alamos NM 87545 USA;
Joint Inst Nucl Astrophys Notre Dame IN 46556 USA;
Univ Victoria Dept Phys &
Astron Victoria BC V8P 5C2 Canada;
Joint Inst Nucl Astrophys Notre Dame IN 46556 USA;
Univ Victoria Dept Phys &
Astron Victoria BC V8P 5C2 Canada;
Hungarian Acad Sci Res Ctr Astron &
Earth Sci Konkoly Observ Konkoly Thege Miklos Ut 15-17 H-1121 Budapest Hungary;
Australian Natl Univ Res Sch Astron &
Astrophys Weston ACT 2611 Australia;
Univ Chicago Dept Geophys Sci Chicago IL 60637 USA;
LANL Computat Phys &
Methods CCS 2 Los Alamos NM 87545 USA;
Hungarian Acad Sci Res Ctr Astron &
Earth Sci Konkoly Observ Konkoly Thege Miklos Ut 15-17 H-1121 Budapest Hungary;
LANL Computat Phys &
Methods CCS 2 Los Alamos NM 87545 USA;
Joint Inst Nucl Astrophys Notre Dame IN 46556 USA;
Osserv Astron Torino Turin Italy;
Arizona State Univ SESE POB 871404 Tempe AZ 85287 USA;
nuclear reactions; nucleosynthesis; abundances; stars: abundances; stars: evolution; stars: interiors;
机译:Nugrid Stellar数据集。 I.恒星从H到BI的恒星,金属Z = 0.02和Z = 0.01
机译:远距晕星的深SDSS光谱学-I.大气参数和恒星金属度分布
机译:尘埃驱动的恒星质量损失与恒星参数的关系-I.太阳金属风模型网格(勘误)
机译:旋转第一星的恒星产量:弱超新星的产量和碳增强超金属差恒星的丰富
机译:z处的恒星形成星系的性质[近似值] 2:运动学,恒星族和金属性。
机译:麦哲伦云。十六。红外星和恒星演化
机译:NuGrid恒星数据集。 I.对于具有金属度Z = 0.02和Z = 0.01的恒星,恒星从H到Bi的产率