Lower main-sequence stars fundamental param.
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/04fc2884-1366-5705-aa6d-9adcd400ec34
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We derive an empirical effective temperature and bolometric luminosity calibration for G and K dwarfs, by applying our own implementation of the Infrared Flux Method to...
