机译:改进的Ni i log(gf)值和金属穷星HD 84937的照片中的值和丰度确定
Department of Physics University of Wisconsin Madison WI 53706 USA;
Department of Physics University of Wisconsin Madison WI 53706 USA;
Department of Astronomy and McDonald Observatory University of Texas Austin TX 78712 USA;
Homer L. Dodge Department of Physics and Astronomy University of Oklahoma Norman OK 73019 USA;
atomic data; methods: laboratory: atomic; stars: abundances; stars: individual (HD 84937); Sun: abundances;
机译:改进的Ni i log(gf)值和金属穷星HD 84937的照片中的值和丰度确定
机译:改进的Vii log(gf)值,超精细结构常数以及太阳和贫金属星HD 84937的光球中的丰度测定
机译:改进的v i log(gf)值在太阳和金属差星HD 84937的照片中的值和丰度确定
机译:金属贫恒星中的锂同位素丰度:与底座/ HDS的观察
机译:化学富集的历史和早期核合成的位点:银河碳贫金属星的CNO丰度
机译:太阳和贫金属星HD 84937的光球中改善的Cr II log(gf)值和丰度测定
机译:改进了CO IG(GF)值和太阳照相中的值和丰度确定HD 84937