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spectral classification

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spectral classification

In astronomy, classification of stars according to their surface temperature and luminosity, as determined from their spectra. Stars are assigned a spectral type (or class) denoted by the letters O, B, A, F, G, K, and M, where O stars (about 40,000 K/39,700°C/71,500°F) are the hottest and M stars (about 3,000 K/2,700°C/5,000°F) are the coolest.

Each letter may be further divided into ten subtypes, B0, B1, B2, and so on. Stars are also assigned a luminosity class denoted by a Roman numeral attached to the spectral type: I (supergiants), II (bright giants), III (giants), IV (subgiants), V (main sequence), VI (subdwarfs), or VII (white dwarfs). The Sun is classified as type G2V. See also Hertzsprung-Russell diagram.



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This approach, based on watershed, is composed of a spectral classification to obtain the markers and a vectorial gradient which gives the spatial information.
The objective of the project was to determine minimum masses and individual spectral classifications for the two stars in HD100213.
The group's 17th session gets under way at Burbage Visitor Centre on Tuesday, September 5, with a presentation by David Conner, of Leicester Astronomical Society, on the spectral classification of stars.
 
 
 
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