A super-AGB star is a star with a mass intermediate between those that end their lives as a white dwarf and those that end with a core collapse supernova, and properties intermediate between asymptotic giant branch (AGB) stars and red supergiants. They have initial masses of 7.5–9.25 M☉ in stellar-evolutionary models, but have exhausted their core hydrogen and helium, left the main sequence, and expanded to become large, cool, and luminous.
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rdfs:label
| - 초점근거성 (ko)
- Super-AGB star (en)
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| - A super-AGB star is a star with a mass intermediate between those that end their lives as a white dwarf and those that end with a core collapse supernova, and properties intermediate between asymptotic giant branch (AGB) stars and red supergiants. They have initial masses of 7.5–9.25 M☉ in stellar-evolutionary models, but have exhausted their core hydrogen and helium, left the main sequence, and expanded to become large, cool, and luminous. (en)
- 초점근거성(영어: Super-AGB star)이란 점근거성가지와 적색 초거성의 중간 성질이 나타나는 항성이다. 백색왜성으로 일생의 끝을 맺는 항성과 중심핵 붕괴 초신성으로 끝을 맞이하는 항성 중간형의 진화 과정에서 나타난다. 항성 진화 모형에 따르면 이들은 처음에 질량이 7.5~9.25M☉이었지만, 주계열을 떠난 후 핵의 수소와 헬륨이 고갈되어 크게 부풀어오르며 표면이 차가워지고 밝아진 상태다. (ko)
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| - A super-AGB star is a star with a mass intermediate between those that end their lives as a white dwarf and those that end with a core collapse supernova, and properties intermediate between asymptotic giant branch (AGB) stars and red supergiants. They have initial masses of 7.5–9.25 M☉ in stellar-evolutionary models, but have exhausted their core hydrogen and helium, left the main sequence, and expanded to become large, cool, and luminous. (en)
- 초점근거성(영어: Super-AGB star)이란 점근거성가지와 적색 초거성의 중간 성질이 나타나는 항성이다. 백색왜성으로 일생의 끝을 맺는 항성과 중심핵 붕괴 초신성으로 끝을 맞이하는 항성 중간형의 진화 과정에서 나타난다. 항성 진화 모형에 따르면 이들은 처음에 질량이 7.5~9.25M☉이었지만, 주계열을 떠난 후 핵의 수소와 헬륨이 고갈되어 크게 부풀어오르며 표면이 차가워지고 밝아진 상태다. (ko)
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