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排序方式: 共有386条查询结果,搜索用时 15 毫秒
1.
Aprajita Verma Vassilis Charmandaris Ulrich Klaas Dieter Lutz Martin Haas 《Space Science Reviews》2005,119(1-4):355-407
Some of the most ‘active’ galaxies in the Universe are obscured by large quantities of dust and emit a substantial fraction
of their bolometric luminosity in the infrared. Observations of these infrared luminous galaxies with the Infrared Space Observatory
(ISO) have provided a relatively unabsorbed view to the sources fuelling this active emission. The improved sensitivity, spatial
resolution and spectroscopic capability of ISO over its predecessor Infrared Astronomical Satellite (IRAS) of enabled significant
advances in the understanding of the infrared properties of active galaxies. ISO surveyed a wide range of active galaxies
which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing
a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many
nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines
as well as broad band features in the mid- and far-infrared. This was particularly useful, since it resulted in the understanding
of the power production, excitation and fuelling mechanisms in the nuclei of active galaxies including the intriguing but
so far elusive ultraluminous infrared galaxies. Detailed studies of various classes of AGN and quasars greatly improved our
understanding of the unification scenario. Far-infrared imaging and photometry revealed the presence of a new very cold dust
component in galaxies and furthered our knowledge of the far-infrared properties of faint starbursts, ULIGs and quasars. We
summarise almost nine years of key results based on ISO data spanning the full range of luminosity and type of active galaxies. 相似文献
2.
The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest
dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006.
We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe)
and others of which there are always many, like meteors and molecules, black holes and binaries. 相似文献
3.
4.
5.
用于棘轮变形预测的棘轮演化统一模型研究 总被引:7,自引:2,他引:7
在大量单轴棘轮实验基础上,研究了均值、幅值、峰值和谷值应力对 304不锈钢的饱和棘轮应变的影响规律,首次提出了棘轮应力σr和棘轮门槛值σrth 的概念,建立了基于单参数控制的、用于饱和棘轮应变预测的 SRM饱和棘轮本构模型和用于独立循环应力工况下棘轮应变演化预测的 REM棘轮演化模型,并由此发展了全面描述任意循环应力工况下棘轮应变演化规律的 URM棘轮演化统一模型。抛物律模型 SRM和幂律模型 REM对实验数据拟合的相关系数均超过 0.98。URM建模容易,只需 4~ 6个试样的单轴棘轮实验数据。此外还讨论了获得 SRM本构模型的单试样实验法。 相似文献
6.
在几何不可调的二元外压式斜板进气道的设计中,选择合理的斜板和唇口几何能数是最重要的问题之一。本文对一个设计马赫数为1.8的这类进气道的斜板和唇口参数进行了风洞试验研究。用缩尺模型风洞试验,对比分析了不同斜板角和不同外侧唇口内唇角,唇缘半径对进气道内流特性的影响,结果表明,对确定的进气道布局,斜板角小的变化对进气道超音速内流总压恢复系数,稳态出口流场周向畸变指数及喘振裕度的影响很大,唇口参数小的改变 相似文献
7.
数控展成电解加工的阴极结构及流场研究 总被引:1,自引:0,他引:1
介绍了应用数控展成电解在整体叶轮毛坯上开槽时的流场特点,讨论了阴极结构对加工间隙内流场的影响规律,并相应对阴极的结构设计提出了一些建议。 相似文献
8.
数控展成电解磨削整体叶轮叶片的过切误差分析及解决方案 总被引:1,自引:0,他引:1
分析了平行直纹展成电解磨削整体叶轮叶片的过切误差,得到了过切误差计算公式,提出了用圆锥磨轮和组合式五轴联动数控方案来消除过切误差的方法。 相似文献
9.
化学镀镍钨磷合金过程中的析氢行为和沉积机理 总被引:1,自引:0,他引:1
本文研究了化学镀镍钨磷合金过程中的析氢行为,发现总析氢量大于金属沉积的量,即产生氢气的法拉第电流大于金属沉积的法拉第电流。认为镍钨磷合金化学沉积的机理是镍、钨、磷、氢的竞争放电,且除金属沉积时伴随着等量的析氢外,氢也能单独析出。温度、pH值和亚磷酸根浓度对合金沉积速度和合金成分的影响表明,该体系能在很宽的工艺范围内获得光亮、均匀、结合力良好的镀层。用塔菲尔斜率分析法测量的合金沉积速度与重量法测得的相一致,说明电化学方法可以用于确定化学度的沉积速度。 相似文献
10.
T. Sbarrato L. Foschini G. Ghisellini F. Tavecchio 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2011
The γ-ray emission of blazar jets shows a pronounced variability and this feature provides limits to the size and to the speed of the emitting region. We study the γ-ray variability of bright blazars using data from the first 18 months of activity of the Large Area Telescope on the Fermi Gamma-Ray Space Telescope. From the daily light-curves of the blazars characterized by a remarkable activity, we firstly determine the minimum variability time-scale, giving an upper limit for the size of the emitting region of the sources, assumed to be spheroidal blobs in relativistic motion. These regions must be smaller than ∼10−3 parsec. Another interesting time-scale is the duration of the outbursts. We conclude that they cannot correspond to radiation produced by a single blob moving relativistically along the jet, but they are either the signature of emission from a standing shock extracting energy from a modulated jet, or the superposition of a number of flares occurring on a shorter time-scale. We also derive lower limits on the bulk Lorentz factor needed to make the emitting region transparent for gamma-rays interacting through photon–photon collisions. 相似文献