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Cooling and energy loss of partially ionized hydrogen gas behind a shock wave
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作者 Oksana Mikhailovna Belova konstantin veniaminovich bychkov 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2018年第8期111-116,共6页
We studied the difference in behavior of total energy and its thermal component during the radiative cooling of partially ionized hydrogen gas. Our calculations were fulfilled for the conditions in the atmosphere of a... We studied the difference in behavior of total energy and its thermal component during the radiative cooling of partially ionized hydrogen gas. Our calculations were fulfilled for the conditions in the atmosphere of a cool star. It is shown that the attenuation of total energy loss does not interfere with the cooling rate. 展开更多
关键词 stellar atmospheres shock wave
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