Stars of later spectral classes from the FBS survey. Preliminary data for seven special cases

Preliminary data are presented on seven “special” objects found in low-dispersion spectral plates of the FBS survey. The first object, FBS 0250+167, is found to be a class M7 dwarf with a high proper motion (∼5.130 arcsec/year) lying about 3 pc from the sun. Three of the objects, with spectra of classes M8–M9, are suspected of being long-period Mirids with large mass losses and surrounded by dense clouds. The three remaining objects have very short low-dispersion spectra on the FBS survey plates (clearly they are non stellar objects) and are of interest for later detailed study. __________ Translated from Astrofizika, Vol. 50, No. 1, pp. 73–85 (February 2007).     

疏散星团NGC2244天区恒星的绝对自行研究

利用上海天文台相隔35年的两期照相底片资料,测定了疏散星团NGC2244所在天区55’×55’范围内495颗恒星基于Tycho-2星表的位置和绝对自行,并对自行精度作了初步分析。     

Effective Hamiltonian for the D'Alembert Planetary Model Near a Spin/Orbit Resonance

The D'Alembert model for the spin/orbit problem in celestial mechanics is considered. Using a Hamiltonian formalism, it is shown that in a small neighborhood of a p:q spin/orbit resonance with (p,q) different from (1,1) and (2,1) the 'effective' D'Alembert Hamiltonian is a completely integrable system with phase space foliated by maximal invariant curves; instead, in a small neighborhood of a p:q spin/orbit resonance with (p,q) equal to (1,1) or (2,1) the 'effective' D'Alembert Hamiltonian has a phase portrait similar to that of the standard pendulum (elliptic and hyperbolic equilibria, separatrices, invariant curves of different homotopy). A fast averaging with respect to the 'mean anomaly' is also performed (by means of Nekhoroshev techniques) showing that, up to exponentially small terms, the resonant D'Alembert Hamiltonian is described by a two-degrees-of-freedom, properly degenerate Hamiltonian having the lowest order terms corresponding to the 'effective' Hamiltonian mentioned above.     

Analysis of the three-dimensional stellar velocity field using vector spherical functions

We apply vector spherical functions to problems of stellar kinematics. Using these functions allows all of the systematic components in the stellar velocity field to be revealed without being attached to a specific physical model. Comparison of the theoretical decomposition coefficients of the equations for a particular kinematical model with observational data can provide precise information about whether the model is compatible with the observations and can reveal systematic components that are not described by this model. The formalism of vector spherical functions is particularly well suited for analyzing the present and future (e.g., GAIA) catalogs containing all three velocity vector components: the propermotions in both coordinates and the radial velocity. We show that there are systematic components in the proper motions of Hipparcos stars that cannot be interpreted in terms of the linear Ogorodnikov-Milne model. The same result is also confirmed by an analysis of the radial velocities for these stars.     

河北舍女寺油田女12—女20断块孔二段沉积微相与油气聚集关系研究

黄骅坳陷南部舍女寺油田的古近系孔店组是在断陷盆地的快速充填过程中形成的典型的河流—三角洲沉积。根据取芯井段的取芯和测井资料分析,把剖面结构、砂体几何形态、沉积构造等微相特征进行描述和分析,划分出水下分流河道、河口坝、席状砂等储层沉积微相类型。研究表明,舍女寺地区沉积微相不仅控制储集层的分布,而且控制油气聚集。研究区中较大厚度的油层分布在水下分流河道的中心部位,即该区沉积微相带的主体部位起着油层控制作用。在复杂断块高含水开发中后期,微突起、微断层、微断鼻等圈闭和储集层的有利配置区,尤其是中心微相带与有利的微构造部位叠合区将是有利高产井区。     

施密特巡天星表的现状和展望

扼要介绍了施密特巡天底片及基于此编制而成的施密特巡天星表的发展历程,并详细介绍了GSC2.3和USNO-B1.0的情况.分析研究了这类星表存在的问题和原因所在,并提出了一个新的计划:利用现有施密特底片资料并增加新的第3期观测,编制一个具有绝对自行、多色测光、系统均匀的高密度全天星表以满足各方面的需要.     

石斑鱼鱼虱病的研究 Ⅴ.盐度对南海鱼虱存活的影响

记述了盐度对南海鱼虱CaligusnanhaiensisWu＆Pan不同发育期的影响。在盐度为10以上时,南海鱼虱的幼虫和成虫对盐度的变化有较大的忍耐性,盐度在10—40之间对幼虫和成虫存活没有明显的影响,24h的实验表明,存活率均为100％。然而,虫卵对盐度的变化较为敏感,虫卵孵化的最适盐度范围为20—35,超出此范围虫卵孵化受到影响。当盐度为10时,虽然孵化率可达100％,但孵出的幼虫活动能力差,多数附着于卵囊上而不能正常活动,不久即死亡。盐度为40时,卵子几乎不能孵化。在淡水中,虫卵、幼虫和成虫均不能正常生存。     

关于干旱监测评估指标的一种新探讨

从有效降水过程观点入手,针对降水过程次数、降水过程总量,尤其是降水过程的时间分布结构和效能,提出了一种新的干旱指数式。该结果在干旱研究分析、监测评估业务和决策服务中都有实用意义。     

福建泉州湾贝类养殖容量评估

通过对泉州湾叶绿素a、初级生产力、生态效率、浮游植物有机碳含量、养殖贝类有机碳含量及其含壳重与鲜组织重比值、潮间带和潮下带及吊养区附着滤食性动物现存量等的调查和检测,应用营养动态模型、沿岸能流模型估算贝类生态容量及扣除野生滤食性动物现存量来估算贝类养殖容量。还采用方建光模型估算贝类养殖容量,并采用统计分析法估算贝类及其各品种的适养面积。3种模型估算的贝类养殖容量分别为43 171t、220 991×104个,46 388 t、237 464×104个,44 049t、225 490×104个。贝类适养总面积为2 878hm2,其中牡蛎Ostrea1 349hm2,缢蛏Sinoncvacula con-stricta1 268 hm2,菲律宾蛤仔Ruditapes philippinarum117hm2,翡翠贻贝Perna viridis144hm2。1999年实际养殖面积2 615 hm2,尚有263 hm2可扩大养殖面积。还讨论了模型的实用性等问题。     

淤泥质潮滩剖面冲淤演变数值模拟分析——以河北省沧州市为例

为全面剖析淤泥质潮滩变化规律及演变特征,运用修改后的输沙公式建立了淤泥质潮滩演变数值模型。经2000,2007年野外实测数据验证,表明该模型各参数设置准确,较真实地反演了滩涂剖面变化过程,可用于淤泥质潮滩的模拟计算。根据数值模型计算结果得出如下结论:1987-2010年河北省沧州市淤泥质潮滩坡度不断增大,但增长速率变化不大,为0.002×10-3。0 m等深线上部坡度逐渐变缓,年均降低0.021×10-3;下部坡度不断变陡,年均增长0.022×10-3。研究区潮滩未达平衡状态,其坡度将进一步变陡。该输沙模型及研究结论对淤泥质潮滩的保护具有重要的理论指导意义,为其科学开发管理提供实际参考依据。