TM923.07 95031439体育照明光色参数现场测试方法的研究=A studyof measuring method for chromaticity param-eter of sport lighting[刊,中]/龚晓斌(中国测试技术研究院)∥计量学报.—1994,15(4).—255—257给出了一种体育照明现场实...TM923.07 95031439体育照明光色参数现场测试方法的研究=A studyof measuring method for chromaticity param-eter of sport lighting[刊,中]/龚晓斌(中国测试技术研究院)∥计量学报.—1994,15(4).—255—257给出了一种体育照明现场实时测量的方法.对国内的数十个大型体育场馆进行了测试评价。展开更多
O432.3 98052818光谱测色仪器的色品精度要求及检测方法=Chro-maticity precision demand and detection meth-ods of the spectrophotometer[刊,中]/侯民贤,赵田冬,叶关荣(浙江大学现代光学仪器国家重点实验室。浙江,杭州(310027))∥...O432.3 98052818光谱测色仪器的色品精度要求及检测方法=Chro-maticity precision demand and detection meth-ods of the spectrophotometer[刊,中]/侯民贤,赵田冬,叶关荣(浙江大学现代光学仪器国家重点实验室。浙江,杭州(310027))∥中国照明电器。—1997,(5)。—1—5从电光源光色参数检测要求出发。讨论了光谱测色仪器的光学系统设计。波长不确定度以及色品坐标不确定度等基本要求及基检测方法。图8参3(方舟)展开更多
In this work, predictions of the spectral energy distribution from populations of single and binary stars are incorporated into a galactic chemical and color evolution model to explore the significance of the effects ...In this work, predictions of the spectral energy distribution from populations of single and binary stars are incorporated into a galactic chemical and color evolution model to explore the significance of the effects of the binary interactions on the color evolution of M33. We first constructed a model without binary interactions, and the model is able to reproduce most of the available observational constraints on the distribution of stellar parameters. We then run simulations with the same set of model parameters but with binary interactions considered. By comparing the results for the populations with and without binary interactions, we find that the inclusion of binary interactions makes the surface brightness greater (~0.1 mag arcsec 2) in FUV-band but smaller (~0.7 mag arcsec 2) in K-band, while it results in the FUV K color bluer (~0.8 mag). To reproduce the observations, a model that considers the binary interactions should make more gas fall onto the disk in the early time of the galaxy evolution, or increase the total stellar mass, or both.展开更多
文摘TM923.07 95031439体育照明光色参数现场测试方法的研究=A studyof measuring method for chromaticity param-eter of sport lighting[刊,中]/龚晓斌(中国测试技术研究院)∥计量学报.—1994,15(4).—255—257给出了一种体育照明现场实时测量的方法.对国内的数十个大型体育场馆进行了测试评价。
文摘O432.3 98052818光谱测色仪器的色品精度要求及检测方法=Chro-maticity precision demand and detection meth-ods of the spectrophotometer[刊,中]/侯民贤,赵田冬,叶关荣(浙江大学现代光学仪器国家重点实验室。浙江,杭州(310027))∥中国照明电器。—1997,(5)。—1—5从电光源光色参数检测要求出发。讨论了光谱测色仪器的光学系统设计。波长不确定度以及色品坐标不确定度等基本要求及基检测方法。图8参3(方舟)
基金supported by the National Natural Science Foundation of China (Grant Nos. 11033008 and 10821061)the Chinese Academy of Sciences (Grant No. KJCX2-YW-T24)
文摘In this work, predictions of the spectral energy distribution from populations of single and binary stars are incorporated into a galactic chemical and color evolution model to explore the significance of the effects of the binary interactions on the color evolution of M33. We first constructed a model without binary interactions, and the model is able to reproduce most of the available observational constraints on the distribution of stellar parameters. We then run simulations with the same set of model parameters but with binary interactions considered. By comparing the results for the populations with and without binary interactions, we find that the inclusion of binary interactions makes the surface brightness greater (~0.1 mag arcsec 2) in FUV-band but smaller (~0.7 mag arcsec 2) in K-band, while it results in the FUV K color bluer (~0.8 mag). To reproduce the observations, a model that considers the binary interactions should make more gas fall onto the disk in the early time of the galaxy evolution, or increase the total stellar mass, or both.
