Proper motions of 59 766 stars absolutized using galaxies in 149 sky fields (PUL2)

The PUL2 catalog has been photographically compiled in Pulkovo according to Deutch's plan. The catalog contains the mean coordinates of stars in the ICRS system at epoch J2000.0 and their original absolute proper motions. The photographic observations were performed with a normal astrograph. The first and second epochs of the photographic plates are 1937–1965 and 1969–1986, respectively. The PUL2 fields uniformly cover the northern sky. The mean difference between the epochs is 24 years. At least three pairs of plates are available for each field. There are one-hour and five-minute exposures on all plates. One pair of plates was taken with a diffraction grating. Only bright reference stars were measured on the pairs of plates with a grating. Based on a reduction model with six constants and using faint (\(15\mathop m\limits_. 2\)) reference stars, we determined the relative proper motions of the stars. We used ～700 galaxies for absolutization. The mean errors in the relative proper motions of the PUL2 stars are 5.5 mas yr^?1 (milliarcseconds per year) in μ_α cos δ and 5.9 mas yr^?1 in μ_δ. When using galaxies, the mean absolutization error is 7.9 mas yr^?1 in both coordinates. By comparing the PUL2 and HIPPARCOS catalogs, we determined the components of the residual rotation vector ω for HIPPARCOS relative to the extragalactic (equatorial) coordinate system: ω_x,y,z=(?0.98, ?0.03, ?1.66)±(0.47, 0.38, 0.42) mas yr^?1. The mean error of one absolute proper motion of a bright PUL2 star in external convergence is 9 mas yr^?1 in both coordinates.     

Schmidt survey in the Galactic anticentre direction. 1. Investigation of open clusters

A study of four open clusters in the direction of the Galactic anticentre (l = 186°, b = +2°) is presented. In a field of 8.32 square degrees proper motions and B magnitudes for about 79 000 stars down to 19.5 were determined on Tautenburg Schmidt plates. For more than 15 500 of them U magnitudes down to 17.3 could be obtained. Additionally, OCA Schmidt plates were used to determine V, R magnitudes in a larger field of 24.45 square degrees for 271 000 stars down to V = 18.2. For stars brighter than V = 15.5 an accuracy of about 1.5 mas/yr has been estimated for proper motions. The rms errors of stellar magnitudes and colour indices are 0.09 – 0.12 mag. Several open clusters have been already known in this direction of the sky, e.g. NGC 2168 or M 35 (C 0605+243), NGC 2158 (C 0604+241) and IC 2157 (C 0601+240). Inspecting the plates and analysing the colour-magnitude diagrams and published data, we could identify an additional anonymous cluster C 0605+242 with a projection on the sky near the centre of M 35 but at a larger distance from the Sun. The cluster membership determination was carried out using information on spatial and proper motion distributions of stars in the field. The colour-magnitude diagrams were derived down to the limiting stellar magnitude. For each cluster the interstellar extinction A_v, the diameters of the core and corona, the ages and spatial velocity components (V,W) relative to the LSR in the Y,Z – Galactic directions were determined. The distances to the clusters of 960 pc, 2 600 pc, 2 520 pc and 3 700 pc were obtained for M 35, IC 2157, C 0605+242 and NGC 2158. They show the loci of the clusters in the Local and Perseus spiral arms and at external border of Perseus arm, respectively.     

空间参考系自行系统与地面自行系统

针对地面FK5和空间依巴谷自行系统 ,采用银河系运动学分析方法发现 ,即使考虑了岁差改正的影响 ,两种自行系统之间仍存在很大差异。用建立在FK5系统上的PPM和ACRS自行与依巴谷自行比较 ,发现FK5自行系统内部存在非刚性运动 ;同时无法用VLBI及LLR所测定的岁差改正值来解释FK5与依巴谷自行系统的关系。     

Measurement of the absolute proper motion of M3 and its space motion

We have measured the absolute proper motions of 534 stars in a 1.5° × 1.5° region around the cluster M3, using 14 plates taken with a 40-cm refractor spanning 80 years. 24 stars in the ACT catalogue were used to define the reference frame and the reduction was made using the central overlapping technique. Using the new data, the membership probabilities were redetermined. The mean absolute motion of the cluster was found to be −0.3 ± 0.3 mas/yr in R.A., and −3.1 ± 0.3 mas/yr in declination. Combining the present data with the known distance and radial velocity, the three-dimensional galactic orbit of M3 was calculated for Allen's galactic potential.     

球状星团NGC4147基于依巴谷系统的自行和空间运动

王家骥等［１］曾得到球状星团ＮＧＣ４１４７的绝对自行为（－２．８２±０．４９,２．３７±０．４３）ｍａｓ／ｙｒ．但是,其中所用的参考星表是Ｂｒｏｓｃｈｅ等［２］１９８５年发表的结果,含有ＡＧＫ３星表的系统误差．在Ｄａｕｐｈｏｌｅ等［３］给出的２６个球状星团轨道远银心距（ａｐｏｇａｌａｃｔｉｃｄｉｓｔａｎｃｅ）与金属度［Ｆｅ／Ｈ］的关系图上,ＮＧＣ４１４７处于一个特殊的位置,即按照它的远银距（５２ｋｐｃ）,它的金属度［Ｆｅ／Ｈ］应该大于－２．０,但实际上只有－１．８３［４］．类似的问题在文［１］的…     

两个底片天区的依巴谷星自行

利用上海天文台佘山４０ 厘米折射望远镜拍摄的２ 个底片天区１５ 张照相底片上的３１ 次观测,以ＡＣＴ 星表作为初始参考星表,按中心重叠法进行归算处理,得到了１６ 颗依巴谷星和３８ 颗场星的高精度位置和自行结果,其中依巴谷星的赤经和赤纬标准误差的平均值分别为１０ ．５ ｍａｓ 和７ ．５ ｍａｓ,赤经自行和赤纬自行标准误差的平均值分别为０ ．７０ ｍａｓ／ｙｒ 和０ ．５９ ｍａｓ／ｙｒ     

适度倾斜：中国区域政策之出路

在社会主义市场经济下,探讨中国区域政策的走向有着深远的现实意义。本文从历史分析入手,用大量事实证明了中国区域政策演变的实质就是倾斜度的提高。倾斜度加大虽然促进了中国经济的发展,但同时也带来了一系列问题,对此,作者提出制定中国区域政策必须坚持适度倾斜的原则,开发优势区位潜力。     

三江源区高寒草地载畜量及超载状况分析(英文)

The Three-River Headwaters region in China is an ecological barrier providing environmental protection and regional sustainable development for the mid-stream and downstream areas, which also plays an important role in animal husbandry in China. This study estimated the grassland yield in the Three-River Headwaters region based on MODIS NPP data, and calculated the proper livestock-carrying capacity of the grassland. We analyzed the overgrazing number and its spatial distribution characteristics through data comparison between actual and proper livestock-carrying capacity. The results showed the following:(1) total grassland yield(hay) in the Three-River Headwaters region was 10.96 million tons in 2010 with an average grassland yield of 465.70 kg/hm2(the spatial distribution presents a decreasing trend from the east and southeast to the west and northwest in turn);(2) the proper livestock-carrying capacity in the Three-River Headwaters region is 12.19 million sheep units(hereafter described as "SU"), and the average stocking capacity is 51.27 SU [the proper carrying capacity is above 100 SU/km2in the eastern counties, 60 SU/km2in the central counties(except Madoi County), and 30 SU/km2in the western counties]; and(3) total overgrazing number was 6.52 million SU in the Three-River Headwaters region in 2010, with an average overgrazing ratio of 67.88% and an average overgrazing number of 27.43 SU/km2. A higher overgrazing ratio occurred in Tongde, Xinghai, Yushu, Henan and Zêkog. There was no overgrazing in Zhiduo, Tanggula Township and Darlag, Qumerleb and Madoi. The remainder of the counties had varying degrees of overgrazing.     

沧州区域可持续发展系统研究

基于控制论对沧州区域可持续发展系统进行研究。以沧州区域行政运行图为背景,抽象出一种简单的闭环控制系统模型,并对该模型的输入信号、被控对象、反馈装置、控制器和系统干扰等特征进行理论分析,说明该控制模型与普通控制模型的区别,以及沧州区域可持续发展系统的特点。利用控制系统反馈思想设计了一种数学计算方法,并通过实际统计数据构建评价指标体系、设计评价模型和系统协调性模型等给出沧州未来几年甚至几十年的总体调控建议。     

InSAR技术及其在沧州地面沉降监测中的应用

随着城市建设的飞速发展,地面沉降危害日益显著,常规的测量方法尽管精度高,但是成本高、采样精度低、测量时间周期长,已经无法满足当今社会的要求。合成孔径雷达干涉测量(InSAR)已成为测量地球表面变化极具潜力的技术,它可以大面积的采样、测量时间短,同时成本也很低。沧州地区至2001年沉降中心累计沉降量已达2236mm。文中介绍用合成孔径雷达干涉测量进行沧州地区地面沉降监测的试验,最后利用InSAR的差分技术得到的沧州地区的地面沉降监测结果,并据此得到一些初步认识。