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physical object > natural object > celestial body > star > early star > O star > sdO |
sdO comparison table |
Subject | has spectral type | has surface temperature | has rotation velocity | has color | has symbol | has absorption line | has relative abundance | has lifetime | is a kind of | has definition | has luminosity class |
---|---|---|---|---|---|---|---|---|---|---|---|
O star | O, B, A, and early F | 35000 K | very high | blue-white | He II | rare | 3 to 6 million years | early star | Very hot blue star, whose spectra is dominated by the lines of singly ionized helium (see Pickering series). (Most other lines are from at least doubly ionized elements, though H and He I lines are also present.) O stars are useful because they are found in dust clouds and virtually define the spiral arms. | ||
subdwarf | greater than 1000 Kelvin | sd | star | Late-type object whose observed color and absolute magnitude place it below the Main Sequence. | VI | ||||||
sdO | 35000 K | very high | blue-white | sd | He II | rare | 3 to 6 million years | subdwarf | Subdwarf O star showing few very broad and shallow Balmer lines and a very strong He II 4686 line. | VI |
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