File:HR-diag-no-text-2.svg · Wikimedia Commons · See Wikimedia Commons
特超巨星
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A hypergiant (luminosity class 0, Ia-0 or Ia+) is a very rare type of star that has an extremely high luminosity, mass, size and mass loss because of its extreme stellar winds. The term hypergiant is defined as luminosity class 0 (zero) in the MKK system. However, this is rarely seen in literature or in published spectral classifications, except for specific well-defined groups such as the yellow hypergiants, RSG (red supergiants), or blue B(e) supergiants with emission spectra. More commonly, hypergiants are classed as Ia-0 or Ia+, but red supergiants are rarely assigned these spectral classi
Wikidata facts
- Subclass of
- star
- Image
- VY Canis Hypergiant.jpg
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- Commons category
- Hypergiant stars
- topic's main category
- Category:Hypergiants
Sources (1)
via Wikidata · CC0
Article · 中文
特超巨星(Hypergiant)在約克光譜分類中的光度屬於0(是數字的零,不是字母O),位置在赫羅圖的最上方,是一種具有極高質量與光度的恆星,顯示它們質量流失非常大。
Abstract from DBpedia / Wikipedia · CC BY-SA