恒星光谱分类是天体光谱自动识别中的重要组成部分。
Stellar spectra classification is an indispensable part of any workable automated recognition system of celestial bodies.
恒星表面有效温度是恒星的一个重要物理参量，是恒星光谱差异的决定因素。
The effective temperature of a star is one of the most important parameters, which determine the continuum and spectral lines in the stellar spectrum.
在第十九章我们已了解到，恒星光谱中的红移是恒星背离地球的运动造成的。
In chap. 19 we saw that red shifts in stellar spectra result from motions away from the earth.
在第十九章我们已了解到，恒星光谱中的红移是恒星背离地球的运动造成的。
Inn chap. 19 we saw that red shifts in stellar spectra result from motions away from the earth.
最后，利用恒星光谱作为数据集，实验验证了RSFPA算法的正确性和有效性。
In the end, the RSFPA algorithm is validated by using star spectrum data as experiment data.
在分析不同色温恒星光谱分布特征的基础上，建立恒星光谱模型，计算色温差异引起的恒星定位误差。
In order to analyze the effect of color temperature in star sensor, the model of stellar spectrum was presented in this paper.
Palle说，如果通过捕捉行星的透射光谱来进行这一表述，可能会比尝试捕捉行星大气层反射的恒星星光效果更好。
Pallé says that this characterization will be done best by capturing a planet's transmission spectra rather than by trying to capture starlight reflected by the planet's atmosphere.
Palle说，如果通过捕捉行星的透射光谱来进行这一表述，可能会比尝试捕捉行星大气层反射的恒星星光效果更好。
Pallé says that this characterization will be done best by capturing a planet's transmission spectra rather than by trying to capture starlight reflected by the planet's atmosphere.
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