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- W2945288048 abstract "Unfortunately, the two of the most important features in stellar spectra, the Lyman-α line and the EUV, are the most difficult to observe. The Lyman-α emission line dominates the UV spectra of stars cooler than the Sun. For the Sun, the intrinsic Lyman-α line flux is about equal to the rest of the FUV flux, whereas for an M star like GJ 876 (M4 V) the Lyman-α line flux is more than twice as large as the rest of the FUV and nearly as large as the entire FUV+NUV flux excluding this line (France et al. 2012)." @default.
- W2945288048 created "2019-05-29" @default.
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- W2945288048 date "2019-01-01" @default.
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- W2945288048 title "Reconstructing the Missing Stellar Emission" @default.
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- W2945288048 doi "https://doi.org/10.1007/978-3-030-11452-7_6" @default.
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