Mid-Holocene Climate Variations Recorded by Palaeolake in Marginal Area of East Asian Monsoon： A Multi-proxy Study

Traditionally, the mid-Holocene in most parts of China was thought to be warmer with higher precipitation, resulting from a strong Asian summer monsoon. However, some recent researches have proposed a mid-Holocene drought interval of millennial-scale in East Asian monsoon margin areas. Thus whether mid-Holocene was dry or humid remains an open issue. Here, Zhuyeze palaeolake, the terminal lake of the Shiyang River Drainage lying in Asian monsoon marginal areas, was selected for reconstructing the details of climate variations during the Holocene, especially mid-Holocene, on the basis of a sedimentological analysis. Qingtu Lake (QTL) section of 6.92m depth was taken from Zhuyeze palaeolake. Multi-proxy analysis of QTL section, including grain size, carbonate, TOC, C/N and δ13C of organic matter, was used to document regional climatic changes during 9-3 cal ka B.P. The record shows a major environmental change at 9.0-7.8 cal ka B.P., attributed to a climate trend towards warmth and humidity. This event was followed by a typical regional drought event which occurred during 7.8-7.5 cal ka B.P. And a warm and humid climate prevailed from 7.5 to 5.0 cal ka B.P., attributed to the warm/humid Holocene Optimum in this region. After that, the climate gradually became drier. Moreover, comparison of the climate record from this paper with the summer insolation at 30°N indicates that the climate pattern reflecting the Asian monsoon changes was caused by insolation change.     

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Molecular Gas Distribution around the Supernova Remnant G40.5-0.5

The distribution of dense molecular gas around the supernova remnant G40.5-0.5 has been investigated by radio spectroscopic observations in the CO (J = 1-0) transition. The molecular gas is found to extend over the entire region of G40.5-0.5. A molecular shell, with a diameter of - 26', coincides with the ionized gas as revealed by the cm-radio observations. This coincidence, along with the velocity discontinuity following the shell, provides direct evidence for interaction between the ionized gas and the dense molecular gas. No clear evidence for cosmic-ray acceleration can be identified from this SNR as previously suggested, due to positional uncertainty in relating the SNR shell defined by CO to the EGRET gamma-ray sources, GRO J1904 06, from the gamma-ray observations.     

γ射线脉冲星脉冲位相关系的研究

本文分析γ射线脉冲星最近的观测数据，研究各波段辐射位相的一些关联，它们对于揭示γ射线脉冲星的辐射机制可能有重要的意义，     

The non-synchronous systems among RS CVN stars

An RS CVn star is considered as non-synchronous if its orbital period differs by more than 4% from its photometric period. Of 88 systems examined according to this criterion, 67 are synchronous, 21 are non-synchronous. For the 21 non-synchronous systems, we find their spectral types are most around KO-2 III, that their orbital eccentricities are larger and their chromospheric activity lower than the average level.     

The standard systems of stellar rotation measurements (II)

The limb darkening effect on the measurement of stellar rotation is discussed in this paper. It is shown that this effect plays an important role in the measurement of V_e sin i. In the extreme case with the limb darkening coefficient of 1.0, it may cause a difference up to 17%. As a sequel to paper [1], this work presents the following new explanation for the systematic differences between Slettebak's new and old systems. The main causes of the systematic differences are: (1) The old system made an inadequate twice repeated correction for the limb darkening. (2) Owing to the historical reason, the old system used too large limb darkening coefficients.     

昆仑山口西Ms8.1地震的地壳变形特征

利用全球定位系统1991－2001年及震后4期GPS观测数据。获得了2001年11月14日昆仑山口西地震（Ms8.1)的同震和震后形变运动图像，跨破裂带GPS网最近两点测得的最大同震形变为1.9m左右，而震后4个月断层蠕滑引起的变形约为80mm，破裂带两侧震后变形幅度具有非对称性。南侧震后变形基本是北侧的2－3倍。研究结果显示破裂带南盘在震后向偏东方向有明显移动，预示本次地震后能量的重新分配与积累，根据近几十年以来东昆仑断裂带的大地震由西向东扩展的特点，未来地震有向东迁移的可能。     

γ射线暴的研究进展（Ⅲ）：GRO的最新观测结果及理论模型

介绍了ＣｏｍｐｔｏｎＧＲＯ卫星对Ⅱ暴的最新观测结果。观测表明，γ暴源的空间分布是各向同性但不均匀的。这种分布基本上排除了γ暴起源于银盘内中子星的模型，表明γ暴要么位于展延的银晕里，要么位于宇宙学距离上。     

南流江中上游毛蟹调查初报

对北部湾南流江水系的日本绒螯蟹合浦亚种(Eriocheir japonicus hepu ensis Dai 1900)的形态特征、生态习性、分布状况、捕捞运输、经济价值、资源利用作了阐述,并对如何加强资源保护提出4点建议。