Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,School of Space Science and Physics,Shandong University at Weihai,Weihai 264209,People's Republic of China;
Department of Physics,University of Stellenbosch,Matieland 7602,South Africa;
Department of Physics,University of Stellenbosch,Matieland 7602,South Africa;
Department of Physics,University of Stellenbosch,Matieland 7602,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
iThemba LABS,7129 Somerset West,South Africa;
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,School of Space Science and Physics,Shandong University at Weihai,Weihai 264209,People's Republic of China;
Institute of Nuclear Research of the Hungarian Academy of Sciences(ATOMKI),H-4001 Debrecen,P.O.Box:51,Hungary;
Institute of Nuclear Research of the Hungarian Academy of Sciences(ATOMKI),H-4001 Debrecen,P.O.Box:51,Hungary;
Institute of Nuclear Research of the Hungarian Academy of Sciences(ATOMKI),H-4001 Debrecen,P.O.Box:51,Hungary;
Institute of Nuclear Research of the Hungarian Academy of Sciences(ATOMKI),H-4001 Debrecen,P.O.Box:51,Hungary;
Institute of Nuclear Research of the Hungarian Academy of Sciences(ATOMKI),H-4001 Debrecen,P.O.Box:51,Hungary;
Department of Information Technology,University of Debrecen,Egyetem tér 1,Debrecen,Hungary;
Institut für Strahlenphysik,Helmholtz-Zentrum Dresden-Rossendorf,D-01314 Dresden,Germany;
Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,School of Space Science and Physics,Shandong University at Weihai,Weihai 264209,People's Republic of China;
School of Physics,and SK Lab.of Nucl.Phys. Tech.,Peking University,Beijing 100871,People's Republic of China;
School of Physics,and SK Lab.of Nucl.Phys. Tech.,Peking University,Beijing 100871,People's Republic of China;
School of Physics,and SK Lab.of Nucl.Phys. Tech.,Peking University,Beijing 100871,People's Republic of China;
School of Physics,and SK Lab.of Nucl.Phys. Tech.,Peking University,Beijing 100871,People's Republic of China;
School of Physics,and SK Lab.of Nucl.Phys. Tech.,Peking University,Beijing 100871,People's Republic of China;
School of Physics and Nuclear Energy Engineering,Beihang University,Beijing100191,People's Republic of China;
high spin states; configuration; chiral doublet bands;
机译:A〜80质量区域中手性核的第一个候选物:〜(80)Br
机译:
机译:〜(219)RA中的高自旋光谱:搜索静态Octupole变形核区域的较低质量边界
机译:在〜80大众区域搜索手性核
机译:在质量上与80和140区域相似的高度变形核的光谱研究。
机译:对手性铜(II)复合物的对映选择性评价由新型手性四烯酸配体配位用于通过质谱法与同位素标记的对映异构法相结合的氨基酸
机译:a~80质量区域中手性核的第一个候选物:80 Br
机译:低质量过剩部分的行星神经和风壳的近二元和脉动核的紫外线观察行星神经元HFG的近二进制核1寻找行星结核的二元核紫外线监测不规则变量的行星核和脉络核波多黎各的行星4