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国家自然科学基金(10778701)

作品数:5 被引量:4H指数:1
相关作者:尹红星陈姗姗宋楠王飞格张记成更多>>
相关机构:山东大学更多>>
发文基金:国家自然科学基金更多>>
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Identification of ten new Galactic HII regions被引量:1
2010年
We discovered ten large HII regions in the Sino-German λ6 cm polarization survey of the Galactic plane. They have been identified according to their flat spectral indexes and the high ratio between the 60 μm infrared emission and the λ6 cm emission. The integrated flux densities as well as the sizes of these sources are given at 4800 MHz. Cross-identifications are made with other major radio catalogs.
RUAN GuiPing 1,2 & SHI WeiBin 1,2 1 Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,School of Space Science and Physics,Shandong University at Weihai,Weihai 264209,China
关键词:CONTINUUMREGIONS
Effects of Substrate Temperature on the Properties of Mo-doped ZnO Films Prepared by RF Magnetron Sputtering被引量:3
2009年
Transparent conducting molybdenum-doped zinc oxide (MZO) films were successfully prepared by radio frequency (RF) magnetron sputtering method on glass substrates under different substrate temperatures. The nature of MZO film is polycrystalline with hexagonal structure and a preferred orientation along c-axis. With increasing substrate temperature from room temperature to 400℃, the crystallinity of the films is deteriorated and the resistivity increases sharply due to both the decrease of carrier concentration and Hall mobility. The lowest resistivity achieved is 9.2×10^-4 Ω· cm with a high Hall mobility of 30 cm^2·V^-1·s^-1 for the film deposited at room temperature. The average transmttance in the visible range exceeds 85% for all the samples. The optical band gap decreases from 3.30 to 3.25 eV with substrate temperature from room temperature to 400℃.
Xianwu XiuYuping CaoZhiyong PangShenghao Han
关键词:MOLYBDENUM
小行星初轨计算的Fortran程序设计
2010年
由改进的Laplace和Gauss方法分别给出小行星初轨计算的程序,通过两程序的比较测试得出结论——两方法适用于三次长时间间隔的角观测资料。为实现一天内角观测资料的小行星初轨计算与位置预报,对改进的Laplace方法流程进行了调整。通过增加迭代方程右矩阵的调整,预报结果可用于指导小行星的跟踪观测,文中给出调整后的流程图及预报效果数值验证。
陈姗姗尹红星
关键词:小行星程序设计
太阳系外行星的凌星观测研究
2011年
为对太阳系外行星的物理参数进行更精确估算,利用山东大学威海天文台/威海市天文台的1 m反射望远镜,对7颗已知具有行星系统的恒星:TrES-1、TrES-3、XO-2、WASP-1、WASP-2、WASP-3、HAT-P-7,进行了凌星现象的观测研究.介绍观测和数据处理的基本情况,给出凌星光变曲线结果及由之推算出的一些行星参数.在总结结果并加以分析的同时,展望下一步将进行的更为深入细致的研究.
张记成曹晨宋楠王飞格张晓彤
关键词:光度计
Optical monitoring of the Seyfert galaxy NGC 4151 and possible periodicities in its historical light curve
2014年
We report B, V and R band CCD photometry of the Seyfert galaxy NGC 4151 obtained with the 1.0m telescope at Weihai Observatory of Shandong University and the 1.56 m telescope at Shanghai Astronomical Observatory from 2005 December to 2013 February. Combining all available data from literature, we have constructed a historical light curve from 1910 to 2013 to study the periodicity of the source using three different methods (the Jurkevich method, the Lomb-Scargle periodogram method and the Discrete Correlation Function method). We find possible periods of P1 = 4 ± 0.1,/92 = 7.5 ±0.3 and P3 = 15.9± 0.3 yr.
Di-Fu GuoShao-Ming HuJun TaoHong-Xing YinXu ChenHong-Jian Pan
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