Radius relations for low-metallicity M-dwarf stars
收藏B2FIND2026-04-04 收录
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https://b2find.eudat.eu/dataset/31dcbe3b-7c3b-59ae-b70b-a263dd1ca3b3
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M subdwarfs are low-metallicity M dwarfs that typically inhabit the halo population of the Galaxy. Metallicity controls the opacity of stellar atmospheres; in metal-poor stars,...
