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      nebula
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  星云
    Infrared Radiation of Planetary Nebula NGC 2242
    行星状星云NGC 2242的红外辐射
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    A MODEL FOR HCO~+ LINE EMISSION IN THE YOUNG PLANETARY NEBULA NGC7027
    年青行星状星云NGC7027 HCO~+谱线发射的一个模型
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    From AGB Star to Planetary Nebula
    从AGB星到行星状星云
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    IMAGING OBSERVATION OF CO IN THE PLANETARY NEBULA M1-7,Ml-16 AND VV47
    行星状星云M1-7,M1-16和VV47的CO成图观测
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    Petrological Model for Condensation Process of Solar Nebula:(1) Condensation Genesis of Chondrites
    太阳星云凝聚过程的岩石学模型:(1)球粒陨石的凝聚成因
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  状星云
    Infrared Radiation of Planetary Nebula NGC 2242
    行星状星云NGC 2242的红外辐射
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    A MODEL FOR HCO~+ LINE EMISSION IN THE YOUNG PLANETARY NEBULA NGC7027
    年青行星状星云NGC7027 HCO~+谱线发射的一个模型
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    From AGB Star to Planetary Nebula
    从AGB星到行星状星云
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    IMAGING OBSERVATION OF CO IN THE PLANETARY NEBULA M1-7,Ml-16 AND VV47
    行星状星云M1-7,M1-16和VV47的CO成图观测
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    Spatially Resolved X-ray Photon Index of the Crab Nebula with Chandra Data
    蟹状星云Chandra卫星观测数据的X射线谱分析
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  “nebula”译为未确定词的双语例句
    Mechanic Analysis of Initial Nebula Rotation
    星系旋转起源机理的分析
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    Sometimes hydregen, sodium and nebula lines appeared from 1979 to 1982. From October, 1982 to December, 1983 (final observation) Hα emission line became strong.
    1982年10月出现强H_α发射线,1983年9月出现H_β发射线,1983年12月H_β发射线消失,H_α发射线仍很强。
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    We present H and K s polarimetric images in a ~5′ field of star forming region NGC7538. The polarimetric images reveal the complex structure of infrared nebulosities and clusters of young stars, associated with the bright infrared sources IRS 1 11. The polarization pattern in the IRS 1 3 nebula shows a dominant illumination from deeply embedded source IRS 1. The morphology of the nebula can be modeled by a low extincted bubble enclosed by redder and highly polarized shell.
    介绍恒星形成区NGC7538的H和Ks波段偏振成像的观测结果.近5′视场的偏振图像揭示了与亮红外源IRS111成协的年轻星团和红外星云的复杂结构.IRS13星云的偏振图像表明星云的近红外辐射主要来自对深埋红外源IRS1的反射;
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    Five H 2 knots are detected to the south and east of the IRS 1 3 nebula.
    在IRS13 星云的南边和东边探测到了5 个H2 knots.
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    The Planets Formed Through the Annular Nebula
    行星形成方式的探讨
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  nebula
       A model with a rather small flux of ? = 10-8MSat/ yr and a tenfold depletion of Saturn's disk in gas due to gas scattering from the solar nebula is at one side of this range.
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       Observations of the nebula associated with the WO star in the galaxy IC 1613 are presented.
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       The monochromatic Hα image clearly reveals a giant bipolar shell structure outside the bright nebula S3.
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       Photometric variability and spectral features of the protoplanetary nebula LSII + 34° 26 = V1853 Cyg
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       Line identification and photometric observations of the future planetary nebula IRAS 18 062+2410=V886 Her in 1997-1999
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         A synchronised accumulation technique is used to achieve a resolution of up to 10-13 cm for the oscillating amplitude of a laser interferometer. Such a technique is applied to observe the 60.4 Hz gravitational radiation which is possibly emitted from the pulsar NP 0532 of the Crab Nebula. Present experiments show that no such signal is received.
            本文采用同步积累技术,使激光干涉仪对于微小振动振幅的检测能力达到10~(-13)厘米的水平;运用这一技术对蟹状星云中的NP0532脉冲星可能存在的60.4赫芝引力辐射进行了观测。实验表明:未收到这一信息。
文摘来源
         Forty theories on the origin of the solar system are critically reviewed, especially with regard to the two fundamental problems : source of planetary material and mode of planetary formation. The following conclusions are drawn : planetary material was neither captured by nor expelled from the sun; the whole solar system was formed from a nebula, as postulated by Kant and Laplace, but their nebular theories need revision and development. A nebular disk was formed around the sun, in it pla...
            本文对四十种有关太阳系起源的学说进行了分析、评价,并就形成行星的物质的来源和行星的形成方式这两个问题,提出一些看法.
文摘来源
         In this paper the propagation of low frequency electromagnetic wave with large amplitude in a magnetized plasma is discussed. It is shown that penetration of magnetic-dipole radiation in the medium of the crab nebula seems to be possible.
            本文讨论了大振幅低频电磁波在磁化等离子体中的传播.指出在蟹状星云介质中磁偶极辐射的穿透似乎是可能的.
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