New WR star in M33
收藏B2FIND2026-04-11 收录
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https://b2find.eudat.eu/dataset/4dc784a9-c454-5d6c-ac73-cf52de015f78
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We expect the evolution of massive stars to be strongly influenced by mass loss and hence to be sensitive to metallicity. It should be possible to test this "Conti scenario" be...
