Data Property: starLuminosityClass
http://www.astro.umd.edu/~eshaya/astro-onto/owl/astronomy.owl#starLuminosityClass
Annotations
- comment: "A number of different luminosity classes are distinguished: * I supergiants Ia-0 (hypergiants or extremely luminous supergiants (later addition)), Example: HD 183143 (spectrum is B6-8 Ia-0) Ia (luminous supergiants), Example: Deneb (spectrum is A2Ia) Iab (intermediate luminous supergiants) Ib (less luminous supergiants), Example: Betelgeuse (spectrum is M2Ib) * II bright giants IIa, Example: Scuti (HD 173764) (spectrum is G4 IIa) IIab Example: HR 8752 (spectrum is G0Iab:) IIb, Example: HR 6902 (spectrum is G9 IIb) * III normal giants IIIa, Example: Persei (spectrum is M4 IIIa) IIIab Example: Reticuli (spectrum is M2 IIIab) IIIb, Example: Pollux (spectrum is K2 IIIb) * IV subgiants IVa, Example: Reticuli (spectrum is K1-2 IVa-III) IVb, Example: HR 672 A (spectrum is G0.5 IVb) * V main sequence stars (dwarfs) Va, Example: AD Leonis (spectrum M4Vae) Vb, Example: 85 Pegasi A (spectrum G5 Vb) * VI subdwarfs (rarely used) * VII white dwarfs (rarely used)" (string)
Property Characteristics (and other axioms)
- functional (starLuminosityClass)
Domains
Ranges
- {("I" (string)), ("II" (string)), ("III" (string)), ("IIIa" (string)), ("IIIab" (string)), ("IIIb" (string)), ("IIa" (string)), ("IIab" (string)), ("IIb" (string)), ("IV" (string)), ("IVa" (string)), ("IVb" (string)), ("Ia" (string)), ("Ia-0" (string)), ("Iab" (string)), ("Ib" (string)), ("V" (string)), ("VI" (string)), ("VII" (string)), ("Va" (string)), ("Vb" (string))}