黑体辐射总是一系列发射和吸收过程的综合结果。
Blackbody radiation always is the result of a succession of emission and absorption processes.
落到致密星上的动能只是简单地加热了星的表面，并以黑体辅射的形式再发射出去。
The kinetic energy falling onto the compact star simply heats the surface and is re-radiated as black-body radiation.
回顾了三十多年来蒙特-卡罗法计算黑体空腔发射率的基本思想和主要算法。
Monte-Carlo method using to calculate the effective emissivity of blackbody cavities in the last three decades was reviewed.
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