hypergiant oor Koreaans
hypergiant
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(astronomy) A star that is extremely massive and even more luminous than a supergiant.
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극대거성
en
very rare star with tremendous luminosity and very high rates of mass loss by stellar winds
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Wolf Rayet stars, slash stars, cool slash stars (aka WN10/11), Ofpe, Of+, and Of* stars are not considered hypergiants.
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Because yellow hypergiants are post-red supergiant stars, there is a fairly hard upper limit to their luminosity at around 500,000–750,000 L☉, but blue hypergiants can be much more luminous, sometimes several million L☉.
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The same region of instability extends to include the even more luminous yellow hypergiants, an extremely rare and short-lived class of luminous supergiant.
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Some but not all LBVs show the characteristics of hypergiant spectra at least some of the time, but many authors would exclude all LBVs from the hypergiant class and treat them separately.
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Hypergiants are only created in the largest and densest areas of star formation and because of their short lives, only a small number are known despite their extreme luminosity that allows them to be identified even in neighbouring galaxies.
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It is expected that it will evolve quickly to a hydrogen-free Wolf-Rayet star, possibly with a short time as a blue hypergiant and luminous blue variable.
본 발명은 태양전지용 세정액 조성물로서, 유기알칼리 화합물, 수용성 글리콜에테르 화합물, 과탄산염, 유기인산 또는 그의 염, 및 물을 포함하는 것을 특징으로 하는 세정액 조성물에 관한 것이다.WikiMatrix WikiMatrix
The MK system assigns stars to luminosity classes: Ib for supergiants; Ia for luminous supergiants; and 0 (zero) or Ia+ for hypergiants.
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Because of their high masses, the lifetime of a hypergiant is very short in astronomical timescales: only a few million years compared to around 10 billion years for stars like the Sun.
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