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- W4249792913 abstract "Recent studies (Frenk and White 1980, 1982) of the (x, y, z) and (Π, θ) distributions of the Galactic globular cluster population have given R o = 6.8±0.8 kpc and Π = 51±26 kms −1 for the inner halo. The observations leading to these solutions are well illustrated by the ρ vs. x plot in figure 1 (Clube and Watson (CW), 1979) for the globulars with the best determined data within |l|, |b| < 20°. The independently determined R o value clearly divides the distribution in such a way that most of the objects on the nearside of the G.C. approach the Sun while those on the farside recede, the probability that this arrangement arises by chance from a “stationary” distribution being ~ 0.002." @default.
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- W4249792913 date "1983-01-01" @default.
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- W4249792913 title "Spiral Structure: Density Waves or Material Arms?" @default.
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- W4249792913 doi "https://doi.org/10.1017/s0074180900032757" @default.
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