Stellar Evolution Through the Red Supergiant Phase
Massive stars less massive than ∼30 <inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><msub><mi>M</mi><mo>⊙</mo></msub></semantics></math></inline-formula> evolve into a red supergiant after the main sequence. Given a standard IMF, this means about 80% of a...
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| Váldodahkkit: | , |
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| Materiálatiipa: | Artigo |
| Giella: | Inglês |
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MDPI AG
2025-07-01
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| Ráidu: | Galaxies |
| Fáttát: | |
| Liŋkkat: | https://www.mdpi.com/2075-4434/13/4/81 |
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