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Autor:
Aguirre, F. Cruz, France, K., Nell, N., Kruczek, N., Fleming, B., Hinton, P. C., Ulrich, S., Behr, P. R.
Far ultraviolet (FUV) emission lines from dwarf stars are important driving sources of photochemistry in planetary atmospheres. Properly interpreting spectral features of planetary atmospheres critically depends on the emission of its host star. Whil
Externí odkaz:
http://arxiv.org/abs/2308.04980