Herbig Ae／Be星的尘埃壳层形态研究     

王俊杰  胡景耀 《天体物理学报》1993,13(4):358-366

我们使用Ｋｕｒｕｃｚ恒星大气模型以及黑体模型对２２颗ＨｅｒｂｉｇＡｅ／Ｂｅ星的紫外数据，ＩＲＡＳ观测数据，地面光学及近红外测光数据资料等进行了拟合计算，用能量平衡方法进行了统计分析得出ＨｅｒｂｉｇＡｅ／Ｂｅ星的尘埃壳层为盘状的结论。  相似文献   

Molecular Gas and Dust in the Massive Star Forming Region S 233 IR     

Rui-Qing Mao  Qin Zeng Purple Mountain Observatory  Chinese Academy of Sciences  Nanjing  National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2004,4(5):440-454

The massive star forming region S 233 IR is observed in the molecular lines CO J = 2-1, 3-2, NH3 (1,1), (2,2) and the 870#m dust continuum. Four submillimeter continuum sources, labelled SMM 1-4, are revealed in the 870μm dust emission. The main core, SMM1, is found to be associated with a deeply embedded near infrared cluster in the northeast; while the weaker source SMM2 coincides with a more evolved cluster in the southwest. The best fit spectral energy distribution of SMM1 gives an emissivity of β = 1.6, and temperatures of 32 K and 92 K for the cold- and hot-dust components. An SMM1 core mass of 246 M⊙ and a total mass of 445 M⊙ are estimated from the 870μm dust continuum emission.SMM1 is found to have a temperature gradient decreasing from inside out, indicative of the presence of interior heating sources. The total outflow gas mass as traced by the CO J = 3-2 emission is estimated to be 35 M⊙. Low velocity outflows are also found in the NH3 (1,1) emission. The non-thermal dominant NH3 line width as well as the substantial core mass suggest that the SMM1 core is a “turbulent,massive dense core”, in the process of forming a group or a cluster of stars. The much higher star formation efficiency found in the southwest cluster supports the suggestion that this cluster is more evolved than the northeast one. Large near infrared photometric variations found in the source PCS-IR93, a previously found highly polarized nebulosity, indicate an underlying star showing the FU Orionis type of behavior.  相似文献   

关于奥伯斯佯谬等问题的再讨论     

王家庆 《天文学报》1989,30(2):157-159

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行星际尘埃同位素和Raman分析     

范章云  许胤林 《紫金山天文台台刊》1989,8(2):101-108

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An Observational and Numerical Study on the Topographic Influence on Dust Transport in East Asia          下载免费PDF全文

JIANG Xuegong  CHEN Shoujun 《Acta Meteorologica Sinica》2009,23(5):629-641

Based on observations and numerical simulations, the topographic impacts on dust transport in East Asia were studied. Two regions frequently attacked by dust storms have been confirmed： one is the western part of Inner Mongolia and the southern Mongolia （namely the Mongolia Plateau）, and the other is the Tarim Basin. The most frequent dust storm occurrence area within the first region appears in its hinterland while that of the second one lies in its southern boundary. Moreover, the region from the northeastern edge of the Tibetan Plateau （TP） to the Loess Plateau is attacked by dust storms second frequently. The dust storms frequently occurring over the Mongolia Plateau axe related not only to the abundant sand and dust sources, but also to the special topographic conditions of East Asia. The most significant factor that influences the dust storms forming in the hinterland of the Mongolia Plateau is the canyon low level jet （CLLJ）, which dominates around the southern areas of the Altay-Sayan Mountains with an east-west direction in the beginning of its formation, and is accompanied by significantly enhanced surface wind afterwards. Due to the obstructive effects of the CLLJ, a lot of dust particles carried by the southward down-slope cold air mass would pile up over the southern slope of the Sayan Mountains. Meanwhile, uneven surface conditions are favorable for the dust particles to go up into the upper atmosphere. With the dust particles piling up continuously, a dust layer is formed in the troposphere and can be recognized as a ＇!dust accumulating container＂, which provides abundant dust particles to be transported later to the downstream areas. Additionally, the topographic features of East Asia also exert a great influence on dust transport. Generally, the easterly CLLJ enhances the easterly dust transport. The down-slope air current over the southern Sayan Mountains and the air flow surrounding the TP near its northeastern edge enhance the southward dust transport. Lastly, weather system influences are also examined. The weathers associated with cold fronts frequently appear over the areas of Mongolia and North China in springtime. The cold front system, in general, carries the sand and dust southwards. Among all topographic influencing elements, the rounding effect of the TP is the strongest. Under the combined influences of the cold front and the rounding effect of topography, most sand and dust particles are transported and then deposited over the Loess Plateau.  相似文献   

椭圆星系中的星系际尘埃     

唐雨平 《天文学进展》2008,26(2):139-154

该文总结了近年来椭圆星系中尘埃起源研究中的一些关键问题,包括尘埃大小的分布及其组成、椭圆星系恒星质量损失速率、尘埃的两种加热机制(恒星辐射加热和电子-尘埃碰撞加热),以及由此导致的尘埃温度分布;尘埃的总质量估算;由热离子导致的尘埃破坏速率,以及与此相关联的椭圆星系热气体分布,等等.综合考虑这些因素,作者认为热气体分布对于椭圆星系中尘埃存在和破坏的影响不可忽视,椭圆星系中星系内部恒星质量损失产生尘埃的起源可能占据着非常重要的地位.  相似文献   

城市道路尘埃的磁性特征及其环境意义     

刘振东  杨凌 《地质科技情报》2005,24(3):93-98

城市环境磁性研究表明,道路尘埃中的粗颗粒磁性载体(频率磁化率系数χ′FD＜5%)多为人为源,磁性矿物以单畴和多畴状态的磁铁矿为主,同时含有少量的赤铁矿和其他磁性矿物;细颗粒磁性载体(χ′FD为7%～11%)多为自然源,磁化率较低(小于100×10-8 m3/kg).磁性物质在迁移时往往与粗一级粒径的尘埃颗粒相伴生,磁性参数(如磁化率)和重金属元素(如铅、锌)质量分数之间呈相关关系,它们之间的关系可以用回归分析方法确定.利用电镜分析、因子分析和聚类分析方法可以识别道路尘埃物质的污染源.因此,道路尘埃的磁性特征研究在城市环境评价中具有潜在的重要意义.  相似文献   

关于"冰臼"问题与韩同林先生商榷     

吕一平 《亚热带资源与环境学报》2008,3(1):89-93

跨世纪的"冰臼"与"壶穴"之争,尘埃未定,缘于尚无定论."发现冰臼"却常见于报道.本文根据国内研究冰川的成果就韩同林先生<发现冰臼>书中"冰臼"的定义、表现、成因、分布、"冰臼"遗迹的保存机理、"冰说"理论以及模拟"冰臼"的实验设计的合理性等问题提出质疑.从而阐明了:天坑、天井、冰洞、冰湖不是"冰臼";闽、粤无"冰臼";"冰说"理论不成立的观点.  相似文献   

一颗恒星“即将”诞生     

《地理教学》2009,(9):44-44

气体和尘埃密集的云雾状天体——星云被认为是字宙孕育恒星的“子宫”。一项新研究预测,在距太阳系400光年远的地方,一个新的恒星“即将”诞生。孕育这个恒星的将主要是质量是太阳两倍的暗星云Barnard68。研究表明,这个位于蛇户座的云雾状天体已开始呈现不稳定状态。而一个质量只有它十分之一的星云正在迅速接近并“快要与它相撞”。  相似文献   

遥感在沙尘暴监测领域中的应用     

周波  周楠茵 《测绘与空间地理信息》2017,(6):103-105

沙尘是全球气溶胶系统的主要特征之一,其对地表辐射收支平衡具有显著影响。在过去的几年中,卫星遥感技术已被广泛应用于空气质量监测。本文整理了不同传感器在该领域中的应用,并分析提出了新的理论和方法。文中提供了一份国内外对雾霾监测研究的简要概述,并有针对性地评估了各种方法和经典指数。最后提出一些观点和建议,希望提高遥感在探测全球沙尘暴事件中所起到的作用。  相似文献