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- Q6220 subject Q6864552.
- Q6220 subject Q8823355.
- Q6220 abstract "A subdwarf, sometimes denoted by "sd", is a star with luminosity class VI under the Yerkes spectral classification system. They are defined as stars with luminosity 1.5 to 2 magnitudes lower than that of main-sequence stars of the same spectral type. On an Hertzsprung–Russell diagram subdwarfs appear to lie below the main sequence.The term "subdwarf" was coined by Gerard Kuiper in 1939, to refer to a series of stars with anomalous spectra that were previously labeled as "intermediate white dwarfs".".
- Q6220 wikiPageWikiLink Q101600.
- Q6220 wikiPageWikiLink Q1048535.
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- Q6220 wikiPageWikiLink Q682966.
- Q6220 wikiPageWikiLink Q6864552.
- Q6220 wikiPageWikiLink Q691914.
- Q6220 wikiPageWikiLink Q8823355.
- Q6220 comment "A subdwarf, sometimes denoted by "sd", is a star with luminosity class VI under the Yerkes spectral classification system. They are defined as stars with luminosity 1.5 to 2 magnitudes lower than that of main-sequence stars of the same spectral type.".
- Q6220 label "Subdwarf".