The dynamics of the dwarf-spheroidal (dSph) galaxies in the gravitational field of the Galaxy is investigated with particular reference to their susceptibility to tidal break-up. Based on the observed paucity of the dSphs at small Galactocentric distances, we put forward the hypothesis that subseque
Effect of dark matter on the dynamics and coalescence in galaxy triplets
β Scribed by L.G. Kiseleva; V.V. Orlov
- Publisher
- Elsevier Science
- Year
- 1993
- Tongue
- English
- Weight
- 633 KB
- Volume
- 36
- Category
- Article
- ISSN
- 0083-6656
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