词条 | Stellar populations |
释义 | Stellar populations Table Stellar populations Population I disk population Population II extreme Population I older Population I intermediate Population II halo Population II members gas A-type stars stars of galactic nucleus high-velocity stars with z-velocities \\>30 km/sec subdwarfs young stars associated with the present spiral structure strong-line stars planetary nebulae (planetary nebula) long-period variables with periods \\<250 days and spectral types earlier than M5e globular clusters (globular cluster) supergiants Me dwarfs novae (nova) RR Lyrae stars (RR Lyrae star) with periods \\>0.4 days Cepheids (Cepheid variable) RR Lyrae stars with periods \\<0.4 days T Tauri stars (T Tauri star) weak-line stars galactic clusters of Trumpler's class I average height over galactic plane (parsecs) 120 160 400 700 2,000 average velocity perpendicular to galactic plane z(km/sec) 8 10 17 25 75 axial ratio of spheroidal distribution 100 ? 25? 5 2 concentration toward centre little little strong? strong strong distribution extremely patchy; spiral arms patchy; spiral arms smooth? smooth smooth age (109 years) 0.1 0.1–1.5 1.5–5.0 5.0–6.0 6 total mass (109 suns) 2 5 47 (combined disk and intermediate Population II) 16 See as table: ![]() |
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