Time-dependent evaporation of icy mantles in hot cores   总被引：1，自引：0，他引：1  

Serena Viti  David A. Williams 《Monthly notices of the Royal Astronomical Society》1999,305(4):755-762

  相似文献   

Dust temperature and the submillimetre–radio flux density ratio as a redshift indicator for distant galaxies     

A. W. Blain 《Monthly notices of the Royal Astronomical Society》1999,309(4):955-960

It is difficult to identify the distant galaxies selected in existing submillimetre-wave surveys, because their positions are known at best to only several arcsec. Centimetre-wave VLA observations are required in order to determine positions to subarcsec accuracy, and so to allow reliable optical identifications to be made. Carilli & Yun pointed out that the ratio of the radio to submillimetre-wave flux densities provides a redshift indicator for dusty star-forming galaxies, when compared with the tight correlation between the far-infrared and radio flux densities observed in low-redshift galaxies. This method does provide a useful, albeit imprecise, indication of the distance to a submillimetre-selected galaxy. Unfortunately, it does not provide an unequivocal redshift estimate, as the degeneracy between the effects of increasing the redshift of a galaxy and decreasing its dust temperature is not broken.  相似文献   

The total‐to‐selective extinction ratio determined from near IR photometry of OB stars     

W. Wegner 《Astronomische Nachrichten》2003,324(3):219-237

  相似文献   

Dust in the disk winds from young stars as a source of the circumstellar extinction     

L. V. Tambovtseva  V. P. Grinin 《Astronomy Letters》2008,34(4):231-240

We consider the problem of dust grain survival in the disk winds from T Tauri and Herbig Ae stars. For our analysis, we have chosen a disk wind model in which the gas component of the wind is heated through ambipolar diffusion to a temperature of ～10⁴ K. We show that the heating of dust grains through their collisions with gas atoms is inefficient compared to their heating by stellar radiation and, hence, the grains survive even in the hot wind component. As a result, the disk wind can be opaque to the ultraviolet and optical stellar radiation and is capable of absorbing an appreciable fraction of it. Calculations show that the fraction of the wind-absorbed radiation for T Tauri stars can be from 20 to 40% of the total stellar luminosity at an accretion rate ? _a = 10^?8-10^?6 M _⊙yr^?1. This means that the disk winds from T Tauri stars can play the same role as the puffed-up inner rim in current accretion disk models. In Herbig Ae stars, the inner layers of the disk wind (r ≤ 0.5 AU) are dust-free, since the dust in this region sublimates under the effect of stellar radiation. Therefore, the fraction of the radiation absorbed by the disk wind in this case is considerably smaller and can be comparable to the effect from the puffed-up inner rim only at an accretion rate of the order of or higher than 10^?6 M _⊙yr^?1. Since the disk wind is structurally inhomogeneous, its optical depth toward the observer can be variable, which should be reflected in the photometric activity of young stars. For the same reason, moving shadows from gas and dust streams with a spiral-like shape can be observed in high-angular-resolution circumstellar disk images.  相似文献   

豫西宜阳地区上二叠统孙家沟组古气候特征分析     

祁帅帅  王艳鹏  彭冰柔  张碧云  宁淑媛  刘晓玲  郑德顺 《地质学报》2020,94(12):3803-3818

二叠纪- 三叠纪之交发生了地史上最大规模的生物灭绝事件,该事件可能与当时气候环境的强烈变化有关。前人对该时期较连续的海相地层揭示的古气候研究较为成熟,而对同时期陆相地层的研究缺乏系统性,研究资料需要进一步完善。本文选取豫西宜阳地区上二叠统孙家沟组为研究对象,运用沉积学、矿物学与元素地球化学等方法对该时期的古气候进行恢复,并与同时期陆相地层对比,进而讨论气候变化对该时期生物灭绝的影响。结果表明：①宜阳地区孙家沟组经历了滨湖- 浅湖- 滨湖等亚相的演化过程,其地层中岩相变化、古生物化石缺失、大量的钙质结核及其它沉积构造的出现揭示了孙家沟组的上段气候明显比下段炎热干旱。②元素地球化学指标以及粘土矿物组合的垂向变化等指示了该时期的气候经历了温湿向炎热半干旱- 干旱转变。③宜阳地区孙家沟组的气候指标所得出的结论与其他地区同时期陆相地层古气候的变化基本一致,反映了研究区与同时期全球古气候的变化存在一致性。二叠纪末期温度的骤升、气候极度干旱化以及陆表生态系统遭受毁灭性破坏等因素,可能是导致或加速陆地生物灭绝的主要原因之一。本次研究对该时期气候变化与生物灭绝之间的关系具有一定的指导意义,为探讨全球P- T之交生物灭绝的原因提供新的证据。  相似文献   

Middle Permian organic carbon isotope stratigraphy and the origin of the Kamura Event     

《Gondwana Research》2020

Large carbon cycle perturbations associated with the Middle Permian (Capitanian) mass extinction have been widely reported, but their causes and timing are still in dispute. Low resolution carbon isotope records prior to this event also limit the construction of a Middle Permian chemostratigraphic framework and global or local stratigraphic correlation, and hence limit our understanding of carbon cycle and environmental changes. To investigate these issues, we analyzed the ¹³C_org values from the Middle Permian chert-mudstone sequence (Gufeng Formation) in the Lower Yangtze deep-water basin (South China) and compared them with published records to build a chemostratigraphic scheme and discuss the underlying environmental events. The records show increased δ¹³C_org values from late Kungurian to early Guadalupian, followed by a decrease to the late Wordian/early Capitanian. The early-mid Capitanian was characterized by elevated δ¹³C_org values suggesting the presence of the “Kamura Event”: an interval of heavy positive values seen in the δ¹³C_carb record. We propose that these heavy Capitanian δ¹³C values may be a response to a marked decline in chemical weathering rates on Pangea and associated reduction in carbonate burial, which we show using a biogeochemical model. The subsequent negative δ¹³C excursion seen in some carbonate records, especially in shallower-water sections (and in a muted expression in organic carbon) coincide with the Capitanian mass extinction may be caused by the input of isotopically-light carbon sourced from the terrestrial decomposition of organic matter.  相似文献   

卫星数据和地面观测结合的珠三角地区颗粒物质量浓度统计估算方法     

陈良富  陈水森  钟流举  陶金花  王子峰 《热带地理》2015,35(1):7-12

利用卫星观测的气溶胶光学厚度资料和模式模拟数据,与地面颗粒物观测资料结合,探讨近地面颗粒物质量浓度的估算方法。具体包括：利用区域气侯模式RAMS（Regional Atmospheric Modeling System）模拟的边界层高度对气溶胶光学厚度进行垂直订正,获得近地面颗粒物消光系数;利用模式模拟的相对湿度和颗粒物吸湿增长经验模型对消光系数进行湿度订正,获得近地面颗粒物干消光系数;并基于干消光系数与颗粒物质量浓度地面站点资料建立的统计关系估算获得每个像元的颗粒物质量浓度。利用地面站点观测的颗粒物浓度资料验证表明,基于卫星资料可以获得近地面颗粒物质量浓度,而且细颗粒物质量浓度具有更好的估算精度。  相似文献   

基于CALIPSO星载激光雷达的中国沙尘气溶胶观测   总被引：2，自引：0，他引：2  

徐成鹏  葛觐铭  黄建平  付强  刘华悦  陈斌 《中国沙漠》2014,34(5):1353-1362

基于2006年6月至2012年5月无云条件下CALIPSO星载激光雷达观测资料,分析中国典型地区（塔克拉玛干沙漠、柴达木盆地、戈壁区和华北）沙尘气溶胶分布。结果表明：塔克拉玛干沙漠和戈壁区为沙尘天气发生频率高值区,且前者在各高度层的沙尘发生频率都大于后者。沙尘发生呈季节性分布。塔克拉玛干沙漠在春季沙尘发生频率最大,抬升最高可至10 km,冬季频率最小,高度最低,主要分布在3 km以下。戈壁区在春季沙尘发生频率、抬升高度最大,冬季抬升高度最低,但低层发生频率大于夏、秋两季。在塔克拉玛干沙漠,沙尘光学厚度春季最大约为0.44,冬季最小约为0.17,春,冬季消光系数峰值最大,可达0.25 km^-1,且随高度的递减率大于夏,秋季。在戈壁区和柴达木盆地,沙尘光学厚度春季最大、秋季最小。在华北,沙尘光学厚度春季最大、夏季最小,消光系数在2 km以上春季最大,这主要是由于春季远距离高空传输到华北的沙尘量最多。塔克拉玛干沙漠与柴达木盆地的退偏比为0.2~0.35,戈壁区为0.16~0.28,可能是由于塔克拉玛干沙漠的物质组成与柴达木盆地相同,而与戈壁区不同。华北因低层沙尘与其他气溶胶混合导致退偏振比廓线随高度递增。4个区域对流层上部退偏比全为0.2,表明高空气溶胶可能为来自相同源区的沙尘。  相似文献   

合肥市郊低层大气的激光雷达探测研究   总被引：7，自引：1，他引：6  

袁松  辛雨  周军 《大气科学》2005,29(3):387-395

利用L300米散射激光雷达对合肥市郊大气边界层进行长期系统观测.分析讨论了大气边界层气溶胶消光系数与温度、湿度的关系, 大气边界层气溶胶消光系数垂直分布和时间变化的主要特征, 给出了激光雷达探测的大气边界层高度的统计特征及其与无线电气象探空仪探测大气边界层高度的比较结果.  相似文献   

Evolution of species diversity of Cretaceous radiolarians from high-latitude paleobiochores     

V. S. Vishnevskaya 《Stratigraphy and Geological Correlation》2009,17(2):218-229

Cretaceous radiolarians of the Boreal regions are considered. Their minimal diversity and low abundance are recorded in stratigraphic intervals corresponding to anoxic events. Paleogeographic and ecostratigraphic distribution trends of Cretaceous radiolarians are established for families Heliodiscidae, Prunobrachidae, Pseudoaulophacidae and some others. The most significant turnovers in evolution of radiolarians are confined to the latest Jurassic-earliest Cretaceous, Albian-Cenomanian, Cenomanian-Turonian, terminal Santonian-earliest Campanian transitions and to the terminal Late Cretaceous.  相似文献