Bright giant
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The luminosity class II in the Yerkes spectral classification is given to bright giants. These are stars which straddle the boundary between ordinary giants and supergiants, based on the appearance of their spectra.[1]
Example bright giants
Well known stars which are classified as bright giants include:
- Alpha Carinae (Canopus): a white (A-type) bright giant
- Epsilon Canis Majoris (Adhara): a blue-white (B-type) bright giant
- Omicron Scorpii: a white (A-type) bright giant
- Theta Scorpii (Sargas): a white (F-type) bright giant
- Beta Draconis: a yellow (G-type) bright giant
- Beta Capricorni (Dabih): an orange (K-type) bright giant
- Alpha Herculis (Rasalgethi): a red (M-type) bright giant
- Gamma Canis Majoris (Muliphein) a (B-Type) bright giant
See also
References
- ↑ Abt, Helmut A. (1957). "Line Broadening in High-Luminosity Stars. I. Bright Giants". Astrophysical Journal 126: 503. Bibcode 1957ApJ...126..503A. doi:10.1086/146423.
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This infobox, "Template:Starbox begin", is from Wikipedia. The list of its authors can be seen in its edit history page. The data in this infobox may not agree or state what Wikipedia states. |
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Temperature | {{{8}}} K |
Other designations | |
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References