Application of the Clustering Method in Molecular Dynamics Simulation of the Diffusion Coefficient     

LIU Qingzhi HU Yangdong 《中国海洋大学学报(英文版)》2008,7(1):43-47

Using molecular dynamics （MD） simulation, the diffusion of oxygen, methane, ammonia and carbon dioxide in water was simulated in the canonical NVT ensemble, and the diffusion coefficient was analyzed by the clustering method. By comparing to the conventional method （using the Einstein model） and the differentiation-interval variation method, we found that the results obtained by the clustering method used in this study are more close to the experimental values. This method proved to be more reasonable than the other two methods.  相似文献   

Improved HCN/HNC linelist, model atmospheres and synthetic spectra for WZ Cas     

G. J. Harris  J. Tennyson  B. M. Kaminsky  Ya. V. Pavlenko  H. R. A. Jones 《Monthly notices of the Royal Astronomical Society》2006,367(1):400-406

We build an accurate data base of 5200 HCN and HNC rotation–vibration energy levels, determined from existing laboratory data. 20 000 energy levels in the Harris et al. linelist are assigned approximate quantum numbers. These assignments, lab-determined energy levels and Harris et al. energy levels are incorporated in to a new energy level list. A new linelist is presented, in which frequencies are computed using the lab-determined energy levels where available, and the ab initio energy levels otherwise.
The new linelist is then used to compute new model atmospheres and synthetic spectra for the carbon star WZ Cas. This results in better fit to the spectrum of WZ Cas in which the absorption feature at 3.56 μm is reproduced to a higher degree of accuracy than has previously been possible. We improve the reproduction of HCN absorption features by reducing the abundance of Si to [Si/H]=−0.5 dex, however, the strengths of the Δ v = 2 CS band heads are overpredicted.  相似文献   

Monte Carlo simulations of H₂ formation on stochastically heated grains     

H. M. Cuppen  O. Morata  Eric Herbst 《Monthly notices of the Royal Astronomical Society》2006,367(4):1757-1765

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Peculiarities in the Formation of Molecular Clouds in the Central Regions of Spiral Galaxies     

E. V. Volkov 《Astrophysics》2004,47(3):335-342

The limitations imposed by the shear instability on the formation of gigantic molecular clouds in the central regions of spiral galaxies are examined. The criteria obtained here are illustrated using the example of six galaxies for which the detailed rotation curves are known. The different mechanisms for formation of molecular clouds which apply in the central and edge regions of disk galaxies are evaluated.  相似文献   

New models of interstellar gas–grain chemistry – II. Surface photochemistry in quiescent cores     

Deborah P. Ruffle  Eric Herbst 《Monthly notices of the Royal Astronomical Society》2001,322(4):770-778

The photodissociation of surface species, caused by photons from the cosmic-ray-induced and background interstellar radiation fields, is incorporated into our combined gas-phase and grain-surface chemical models of quiescent dense interstellar cores. For the cores studied here, only cosmic-ray-induced photons are important. We find that photodissociation alters gas-phase and surface abundances mainly at large cloud ages (≳ 10^6–7 yr). The abundances of those surface species, such as H₂O, that are readily reproduced on the surface following photodissociation are not strongly affected at any time. The abundances of surface species that are, on the other hand, reformed slowly via surface reactions possessing activation energy (e.g. CH₃OH) are reduced, while the abundances of associated surface photoproducts (e.g. CO) increase. In the gas phase, inclusion of surface photodissociation tends to increase molecular abundances at late times, slightly improving the agreement with observation for TMC-1.  相似文献   

Monte Carlo simulations of H₂ formation on grains of varying surface roughness     

H. M. Cuppen  Eric Herbst 《Monthly notices of the Royal Astronomical Society》2005,361(2):565-576

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南极沿海伯尔顿盐湖两种越冬浮游动物温度耐性的初步研究          下载免费PDF全文

王自磐 《极地研究》1988,1(2):28-36

本文报导了南极大陆沿海伯尔顿湖两种越冬浮游动物:双刺镰状水蚤和球栉水母的耐热和耐过冷能力的实验.结果表明,两种动物具有较强的温度耐性,其12小时LD_(50)的上、下限温度,雌性双刺镰状水蚤可在14.8℃和—10℃偏下,球栉水母可在13.1℃和—8℃偏下.它们忍受的温度范围大于其他一些南极沿岸海洋无脊椎动物的.这两种动物的耐温能力有明显的季节差异,表明动物具有较强的适应环境温度变化和生理调节能力,这可能是受环境温度自然驯化的结果.  相似文献   

紫金山天文台13.7米望远镜水脉泽观测星表     

韩溥  吴月芳 《紫金山天文台台刊》1995,14(3):184-221

本文简要总结了自1990年8月至1994年1日在紫金山天文台13.7米射电望远镜上进行的水脉泽源的观测,观测结果汇集为表1和图1。在所有435个观测对象中共观测到195个水脉泽源,其中108个为新探测到的 本文对观测仪器和数据处理亦作了简要介绍。  相似文献   

Cep　OB4恒星形成区的IRAS观测     

罗绍光 《中国天文和天体物理学报》1995,(2)

对恒星形成区ＣｅｐＯＢ４的ＩＲＡＳ观测结果的详细分析和研究表明，与年轻星团Ｂｅ５９相联系的分子云物质的原始分布是高度成块的。Ｂｅ５９诞生于一个平均密度为１００─２００ｃｍ（－３）云的背向太阳一侧。强烈的电离辐射以及星风已经在其诞生地产生了一个半径大约为５ｐｃ的＂水泡型（Ｂｌｉｓｔｅｒ）＂电离氢区及与之相关的红外源。电离辐射也穿过云际介质到达与母云分离的另两个云的表面，形成了从侧面看到的电离波前及被压缩和加热的中性物质壳。在这个恒星形成区中，虽然有大量年轻恒星存在，但大质量恒星的形成已经停止。红外发射主要起源于标准尘埃粒子的热平衡发射。但在主激发星团Ｂｅ５９附近的ＨＩＩ区中２５μｍ发射的显著增强可能与某种与电离气体相混合的新型尘埃粒子有关。  相似文献   

Masers in star-forming regions     

R. J. Cohen 《Astrophysics and Space Science》1995,224(1-2):55-62

Maser action in the interstellar medium produces the brightest and most spectacular molecular lines that radio astronomers can study. Strong maser action was first detected in OH (at 1.6 GHz) and water (at 22 GHz) in star-forming regions, but with improvements in mm and submm-wave technology, and improved laboratory data, many new maser transitions are being identified. For methanol alone over 20 maser transitions have been identified in star-forming regions. This review summarizes recent observational developments. Masers provide the most readily detectable indicators of the formation of massive young stars, and offer our best prospect for making a complete census of starforming regions in the Galaxy. Using radio interferometers the structure of the regions can be probed on angular scales of 1 milliarcsecond. The use of masers as probes of the physical conditions in these regions is discussed.  相似文献