Galaxy disruption in a halo of dark matter

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Abstract

The relics of disrupted satellite galaxies have been found around the Milky Way and Andromeda, but direct evidence of a satellite galaxy in the early stages of disruption has remained elusive. We have discovered a dwarf satellite galaxy in the process of being torn apart by gravitational tidal forces as it merges with a larger galaxy's dark matter halo. Our results illustrate the morphological transformation of dwarf galaxies by tidal interaction and the continued buildup of galaxy halos.

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Forbes, D. A., Beasley, M. A., Bekki, K., Brodie, J. P., & Strader, J. (2003). Galaxy disruption in a halo of dark matter. Science, 301(5637), 1217–1219. https://doi.org/10.1126/science.1089237

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