助手标题  
全文文献 工具书 数字 学术定义 翻译助手 学术趋势 更多
查询帮助
意见反馈
   拱星壳 的翻译结果: 查询用时:0.045秒
图标索引 在分类学科中查询
所有学科
更多类别查询

图标索引 历史查询
 

拱星壳
相关语句
  circumstellar shell
     Mark Ⅲ stellar interferometer and Infrared Spacial Interferometer(ISI)have brought a few encouraging results for binary star measurements and circumstellar shell observations.
     美国Mark Ⅲ恒星干涉仪和红外干涉仪ISI已经在双星和拱星壳的观测方面取得了令人鼓舞的观测成果。
短句来源
  circumstellar shells
     DOUBLE-PEAKED SPECTRAL PROFILES OF CIRCUMSTELLAR OH MASER EMISSION AND MULTIPLE DISTINCY AND EXPANDING CIRCUMSTELLAR SHELLS
     拱星OH脉泽辐射频谱的双峰结构和多重分离的膨胀拱星壳
短句来源
     The high resolution imaging technology based on optical interferometry will open up broad prospects for researches in astrophysics. In this paper we comprehensively describe its astrophysical applications, including the studies on stellar physics, binary and multiple stars, quasars and nuclei of galaxies, protoplanetary, circumstellar shells, and et al.
     光学高分辨率干涉测量和成图在天体物理研究方面将具有广阔的应用前景,其中包括恒星物理、双星和多星系统、类星体和星系核、原行星和拱星壳等的研究。
短句来源
  相似匹配句对
     star
    
短句来源
     The Temperature Structure of the Circumstellar Envelopes of Mira Variables
     Mira变包层的温度结构
短句来源
     Gauged Q-stars
     规范Q
短句来源
     The Velocity Fields of Circumstellar Envelop of Mira Variables
     Mira变包层的速度流场
短句来源
     THE OH/IR STARS WITH SiC CIRCUMSTELLAR ENVELOPES
     具有碳化硅层的OH/IR
短句来源
查询“拱星壳”译词为用户自定义的双语例句

    我想查看译文中含有:的双语例句
例句
为了更好的帮助您理解掌握查询词或其译词在地道英语中的实际用法,我们为您准备了出自英文原文的大量英语例句,供您参考。
  circumstellar shell
A high-esolution spectrum in the wavelength range 3600-6700 ? contains both photospheric lines and circumstellar shell lines.
      
An analysis of the radial velocities measured from spectral features originating in the atmosphere and in the circumstellar shell has revealed a high-velocity (~60 km s-1) component of the stellar wind from AFGL 2688.
      
We analyzed the wavelength dependence of extinction in the circumstellar shell outside fadings, which was similar to Whitford's standard reddening law.
      
A tentative evolutionary sequence for carbon stars derived from circumstellar shell parameters
      
These facts strongly support the theory of the photoproduction of OH from H2O induced by ambient interstellar UV photons penetrating the circumstellar shell.
      
更多          
  circumstellar shells
The transfer of polarized radiation in inhomogeneous circumstellar shells with a spheroidal spatial distribution of porous dust particles is computed.
      
The evidence of circumstellar shells for K type stars
      
The results lead to the conclusion that the presence of circumstellar shells seems to be very unlike for these objects in spite of their evolutionary status which is intermediate between M and C type stars.
      
In this paper we investigate the properties of dust in circumstellar shells around very young massive compact IR sources (Becklin-Neugebauer objects).
      
Evidence for the effect of the interstellar far UV-radiation on circumstellar shells
      
更多          


The high resolution imaging technology based on optical interferometry will open up broad prospects for researches in astrophysics. In this paper we comprehensively describe its astrophysical applications, including the studies on stellar physics, binary and multiple stars, quasars and nuclei of galaxies, protoplanetary, circumstellar shells, and et al. Mark Ⅲ stellar interferometer and Infrared Spacial Interferometer(ISI)have brought a few encouraging results for binary star measurements and circumstellar shell...

The high resolution imaging technology based on optical interferometry will open up broad prospects for researches in astrophysics. In this paper we comprehensively describe its astrophysical applications, including the studies on stellar physics, binary and multiple stars, quasars and nuclei of galaxies, protoplanetary, circumstellar shells, and et al. Mark Ⅲ stellar interferometer and Infrared Spacial Interferometer(ISI)have brought a few encouraging results for binary star measurements and circumstellar shell observations. The space astrometric interferometer, POINTS, will be of inestimably benifit to the survey of Cepheid parallax, the determination of masses of stars in binary systems, the study of the Galactic structure and the mass distribution in the Galaxy, and so on. Here, we can only give a brief introduction for potential abilities of optical interferometry and synthesis apertures in the field of astrophysics.

光学高分辨率干涉测量和成图在天体物理研究方面将具有广阔的应用前景,其中包括恒星物理、双星和多星系统、类星体和星系核、原行星和拱星壳等的研究。美国Mark Ⅲ恒星干涉仪和红外干涉仪ISI已经在双星和拱星壳的观测方面取得了令人鼓舞的观测成果。正在研制中的天体测量空间干涉仪POINTS将会为造父视差的测定、双星系统恒星质量的确定、银河系结构和质量分布的研究等带来难以估量的效益。本文仅就上述内容作一简要介绍。

It is important and difficult for the fitting of the infrared spectrum of AGB stars. This is of vital importance to the determination of many physical parameters. In this paper, the double-blackbody model for the infrared spectrum of AGB stars is built, and by using Taylor series method, the difficulty of this complex non-linear model fitting is solved. Taking this fitting method, we get the more accurate color temperatures of the central stars and dust shells of AGB stars, and the more reasonable infrared spectruni...

It is important and difficult for the fitting of the infrared spectrum of AGB stars. This is of vital importance to the determination of many physical parameters. In this paper, the double-blackbody model for the infrared spectrum of AGB stars is built, and by using Taylor series method, the difficulty of this complex non-linear model fitting is solved. Taking this fitting method, we get the more accurate color temperatures of the central stars and dust shells of AGB stars, and the more reasonable infrared spectruni curves.

本文讨论了有拱星壳层的AGB星的红外辐射的双黑体模型并给出了便于拟合某些AGB星的红外观测数据的数学表达式,应用Taylor级数方法解决了这一复杂非线性模型拟合的困难,从而得出了一些AGB星较合理的中心星及壳层的色温度和红外能谱曲线。

Some fitting methods are discussed for the models of the infrared spectra of the late type stars, and the practical fitting method, i.e. the linearization method (Taylor series method) is given for the "double-blackbody model" fitting of the late type stars with circumstellar dust shells. Based on the fitting results and the computer programming, advantages and shortages about the linearization method are also discussed in the paper

本文针对晚型星红外辐射的一些模型,讨论相应的拟合方法。对有拱星壳层的晚型星的双黑体模型,给出了具体的拟合方法──线性化方法。最后我们就拟合结果及拟合程序编制方面讨论了线性化方法的优缺点。

 
<< 更多相关文摘    
图标索引 相关查询

 


 
CNKI小工具
在英文学术搜索中查有关拱星壳的内容
在知识搜索中查有关拱星壳的内容
在数字搜索中查有关拱星壳的内容
在概念知识元中查有关拱星壳的内容
在学术趋势中查有关拱星壳的内容
 
 

CNKI主页设CNKI翻译助手为主页 | 收藏CNKI翻译助手 | 广告服务 | 英文学术搜索
版权图标  2008 CNKI-中国知网
京ICP证040431号 互联网出版许可证 新出网证(京)字008号
北京市公安局海淀分局 备案号:110 1081725
版权图标 2008中国知网(cnki) 中国学术期刊(光盘版)电子杂志社