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- W4210554447 abstract "Galaxies occur in a wide variety of systems ranging from binary pairs through small groups to rich clusters. These systems in turn possess a wide range of densities, with typical separations between bright (L ≫ L * = 3.4 × 10 10 L⊙) galaxies varying from ≲ 10 kpc up to ~ 1 Mpc. Among the most common of these systems are small, loose groups containing ≲ 10 bright galaxies with separations ≳ 100 kpc. Such systems probably contain a substantial fraction of all galaxies (de Vaucouleurs 1975; van den Bergh 1962; Karachentseva 1973). Familiar examples include the Local Group and M81 group." @default.
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- W4210554447 date "1978-01-01" @default.
- W4210554447 modified "2023-09-27" @default.
- W4210554447 title "Optical Studies of Small Groups of Galaxies" @default.
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- W4210554447 doi "https://doi.org/10.1017/s0074180900144213" @default.
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