The pulsating hydrogen-deficient star LSS 3184 (BX Cir)

We present extensive photometry and spectroscopy of the extremely hydrogen-deficient star, LSS 3184, recently discovered to be a rapid variable (period ∼0.1066 d) strikingly similar to V652 Her. Over 95 h of photometry confirms the reported variability, which is of rather low amplitude (Δ V ∼0.03 mag), defines the light curve with greater precision and establishes a much more accurate ephemeris (period ∼0.106 578 4 d) to form a basis for detecting period change. Attention is drawn to the usefulness of a period-finding technique that fits harmonic components to the photometric observations. Spectroscopy shows a peak-to-peak variation in radial velocity of about 30 km s⁻¹, which, when combined with the photometric observations, confirms the pulsational nature of the variability and strongly indicates that the pulsations are radial in nature.     

球上最小二乘问题向后误差的估计

A.N.Malyshev给出了球上最小二乘问题计算解的最佳向后扰动量表达式。从该表达式出发计算最佳向后扰动量却是很困难的。本文给出 1种有效的估算方法 ,所得结果对检验计算解的向后稳定性是有用的。并用几个简单的数值例子验证了所给算法的有效性。     

三种体系萃取分离-液闪测定海水中234Th的比较研究

本文对TOA萃取剂萃取钍适宜的操作条件及萃取溶剂进行了试验,提出了TOA/苯萃取234Th的最佳条件: 在 1cm3含 234Th的 6mol/dm3 HNO3 溶液中,用体积比为 0. 5的TOA/苯溶液 2cm3 萃取,然后用 2cm3 1. 0mol/dm3 H2SO4反萃取,最高萃取率达 94%.对TOA/苯、TBP/煤油和TTA/苯这 3种萃取体系的萃取效率及其影响因素、萃取机理、成本等做了比较,认为 3种体系各有利弊,但均可有效地应用于相关的海洋学研究中.