The Wolf-Rayet Connection - Luminous Blue Variables and Evolved Supergiants
1991 ◽
Vol 143
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pp. 485-498
The physical characteristics and behavior of evolved massive stars in three different mass ranges are reviewed with application to whether they may eventually evolve to the WR stage 1. >40-50 M⊙ as LBV's, 2. ∼30-40 M⊙ as cool hypergiant-OH/IR stars and 3. ∼10-30 M⊙ as red supergiant-OH/IR stars. I emphasize the importance of the relatively short but high mass loss phases as LBV's and as OH/IR stars in determining the fate of massive stars from 10 to 100 M⊙.
2003 ◽
Vol 212
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pp. 38-46
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1989 ◽
Vol 113
◽
pp. 229-240
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1981 ◽
Vol 59
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pp. 293-296
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1989 ◽
Vol 113
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pp. 135-148
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2017 ◽
Vol 375
(2105)
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pp. 20160268
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1999 ◽
Vol 169
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pp. 222-229
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