期刊
KINEMATICS AND PHYSICS OF CELESTIAL BODIES
卷 24, 期 2, 页码 89-98出版社
ALLERTON PRESS INC
DOI: 10.3103/S0884591308020049
关键词
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资金
- DREAM
- NIST
- UVES Paranal Observatory Project
- ESO DDT Program [ID 266, D-5655]
- Research Foundation of the Chungbuk National University, Republic of Korea
- Astrophysical Center of the Sejong University, Republic of Korea
- Swiss National Science Foundation [IB7320-110996]
Absorption lines of some actinides, namely, actinium (Z = 89), protactinium (91), neptunium (93), plutonium (94), americium (95), curium (96), berkelium (97), californium (98), and einsteinium (99), were identified in the spectrum of one of the most peculiar main-sequence stars HD 101065 (Przybylski's star). In the identification we used a high-resolution spectrum (R = 80 000) acquired at the 8.2-m ESO telescope.
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