Properties of Radiative Shock Waves in the Atmospheres of Red Dwarf Stars
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DOI: 10.1007/s10511-019-09577-4
Abstract: The emission from the gas behind the front of a stationary shock wave is calculated for the conditions in the atmospheres of red dwarf stars for velocities u0 from 30 to 100 km/s. Energy exchange… read more here.
Keywords: atmospheres red; red dwarf; emission; dwarf stars ... See more keywords