The central dusty torus in the active nucleus of NGC 1068

Active galactic nuclei (AGNs) display many energetic phenomena--broad emission lines, X-rays, relativistic jets, radio lobes--originating from matter falling onto a supermassive black hole. It is widely accepted that orientation effects play a major role in explaining the observational appearance of AGNs. Seen from certain directions, circum-nuclear dust clouds would block our view of the central powerhouse. Indirect evidence suggests that the dust clouds form a parsec-sized torus-shaped distribution. This explanation, however, remains unproved, as even the largest telescopes have not been able to resolve the dust structures. Here we report interferometric mid-infrared observations that spatially resolve these structures in the galaxy NGC 1068. The observations reveal warm (320 K) dust in a structure 2.1 parsec thick and 3.4 parsec in diameter, surrounding a smaller hot structure. As such a configuration of dust clouds would collapse in a time much shorter than the active phase of the AGN, this observation requires a continual input of kinetic energy to the cloud system from a source coexistent with the AGN.     

MCS-48单片机反汇编程序

本文给出了一个在APPLEⅡ上进行MCS-48系列单片机反汇编程序.     

La_(1-x)Sr_xMnO_3阴极材料的制备及性能

溶胶-凝胶法制备单相性、均匀性较好的La(1-x)SrxMnO3（x=0．1,0．2,0．3,0．4,0．5）纳米微粉系列样品,并用X射线衍射分析样品的结构类型．考察样品的烧结特性和高温电导率随晶粒尺寸的变化规律．通过电池伏安特性曲线的测量,对锰酸锶镧作为（ZrO2）0.92（Y2O3）0.08电解质燃料电池阴极的性能进行研究．     

可降解多氯联苯(PCB_s)菌体的初步实验研究

本文以PCBs为唯一碳源,讨论了无色菌、假单胞菌、肢动胶菌和酿酒酵母菌在不同PCB_s浓度,培养温度下的生成情况,初步得出了上述菌体降解PCB_s的最佳实验条件。