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- W2111587098 abstract "This paper argues that the Milky Way galaxy is probably the largest member of the Local Group. The evidence comes from estimates of the total mass of the Andromeda galaxy (M31) derived from the three-dimensional positions and radial velocities of its satellite galaxies, as well as the projected positions and radial velocities of its distant globular clusters and planetary nebulae. The available data set comprises 10 satellite galaxies, 17 distant globular clusters and nine halo planetary nebulae with radial velocities. We find that the halo of Andromeda has a mass of ∼ together with a scalelength of ∼90 kpc and a predominantly isotropic velocity distribution. For comparison, our earlier estimate for the Milky Way halo is Although the error bars are admittedly large, this suggests that the total mass of M31 is probably less than that of the Milky Way. We verify the robustness of our results to changes in the modelling assumptions and to errors caused by the small size and incompleteness of the data set." @default.
- W2111587098 created "2016-06-24" @default.
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- W2111587098 date "2000-08-21" @default.
- W2111587098 modified "2023-09-27" @default.
- W2111587098 title "The mass of the Andromeda galaxy" @default.
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- W2111587098 doi "https://doi.org/10.1046/j.1365-8711.2000.03645.x" @default.
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