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[93] These could rather evolve to a Wolf–Rayet star, characterised by spectra dominated by emission strains of aspects heavier than hydrogen, which have attained the area resulting from strong convection and rigorous mass loss, or from stripping with the outer layers.[94] Some significant stars, specifically luminous blue variables, are quite https://history-of-judo71592.is-blog.com/42781213/new-step-by-step-map-for-service

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