Subject |
is a kind of |
has spectral type |
has definition |
has hydrogen line strength |
hydrogen-deficient C star | hydrogen-deficient star | F star, G star | A subgroup of high-luminosity C stars with weak or absent hydrogen lines, mostly of types F and G. | weak |
lithium star | C star | G star, M star | Peculiar giant star (spectral types G-M) whose spectra show high abundances of lithium. They are primarily S stars and carbon stars, although Li is also found in T Tauri stars, and is sometimes observed in normal late-type giants. Interstellar Li / H ≈ 2 × 10-10. (Solar system Li / H ≈ 10-9.) Lithium is destroyed rapidly (in about 7500 years) at typical nuclear burning temperatures. Spallation is the only production mechanism known for 6Li, but 7Li can be transported from the core in the form of 7Be and converted in the envelope to 7Li by electron capture. Observed 7Li / 6Li > 10. | |
N star | C star | cooler than G2 | In the old terminology, the cooler C-type stars. | |
R star | C star | cooler than G2 | Star with spectral characteristics similar to those of K stars except that molecular bands of C2, CN, and CH are present instead of TiO bands. | |