K-H_2_ line shapes for cool brown dwarfs spectra
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/d34a9f8e-5192-59a3-b002-67e0d76917c7
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Observations of cooler and cooler brown dwarfs show that the contribution from broadening at many bars pressure is becoming important. The opacity in the red optical to near-IR...
