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Stellar Evolution Through the Red Supergiant Phase

delete2025-08-21
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PRE
AI
S
Sylvia Ekström *
C
C. Georgy
DOI：10.3390-galaxies13040081delete
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摘要

摘要

En 中文
质量小于∼30 M⊙的恒星在主序阶段后演化为红超巨星。根据标准的IMF，这意味着约80%的所有单颗大质量恒星将经历这一阶段。RSGs（红超巨星）以对流为主导，其半径可能延伸至数千倍太阳半径。它们的低温度和低引力使其容易通过脉动驱动的风或质量损失爆发失去大量质量。RSGs是II型（最常见的一种核心坍缩）超新星的母体。在本综述中，我们概述了对大质量恒星演化这一壮观阶段的理论理解。
Keyword:
red supergiant
massive star evolution
mass loss
core-collapse supernovae
convection

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