Equivalent widths of metal-poor stars
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/b16e3613-0898-50d9-879f-e3021a8bba2d
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It is well established that stellar effective temperatures determined from photometry and spectroscopy yield systematically different results. We describe a new, simple method...



