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Cepheid variable

  • n. [天] 造父变星;仙王座δ

专业释义英英释义

  • 造父变星 - 引用次数:1

    参考来源 - 新尘埃模型的分析及其消光影响

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Cepheid variable

  • abstract: A Cepheid ( or ) is a member of a class of very luminous variable stars. The strong direct relationship between a Cepheid variable's luminosity and pulsation period secures for Cepheids their status as important standard candles for establishing the Galactic and extragalactic distance scales.

以上来源于: WordNet

 柯林斯英汉双解大词典 

Cepheid variable /ˈsiːfɪɪd/

  • 1. 

    N any of a class of variable stars with regular cycles of variations in luminosity (most ranging from three to fifty days). There is a relationship between the periods of variation and the absolute magnitudes, which is used for measuring the distance of such stars 造父变星 [astronomy]

双语例句

  • It is the spiral galaxy NGC 4603, the most distant galaxy in which Cepheid variables have been found.

    本图其中一星系漩涡星系ngc 4603,本报告中发现造变星的最远星系。

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  • NASA Hubble Space Telescope (HST) view of the magnificent spiral galaxy NGC 4603, the most distant galaxy in which a special class of pulsating stars called Cepheid variables have been found.

    哈勃太空望远镜(HST)拍摄壮丽的漩涡星系ngc 4603,现今发现一类特殊变星——造父变星最远星系。

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  • This was accomplished by observing Cepheid variables at optical wavelengths out to greater distances than obtained previously and comparing those to similar measurements from ground-based telescopes.

    通过观测先前得多的造父变星的可见光谱实现的,结果地面望远镜观测结论类似

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