Hot subdwarf stars radial velocity variability
收藏B2FIND2026-03-19 收录
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https://b2find.eudat.eu/dataset/82bd7d04-0ce7-58fd-9dbf-a3fa811665b3
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It is generally thought that hot subdwarfs are helium-core- or helium-shell-burning objects with extremely thin hydrogen envelopes and that binary interactions are always needed...
