Two major accretion epochs in M31 from two distinct populations of globular clusters
Two major accretion epochs in M31 from two distinct populations of globular clusters
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London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Contents
Large galaxies grow through the accumulation of dwarf galaxies
1
,
2
. In principle it is possible to trace this growth history via the properties of a galaxy’s stellar halo
3
–
5
. Previous investigations of the galaxy Messier 31 (M31, Andromeda) have shown that outside a galactocentric radius of 25 kiloparsecs the populati...
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Two major accretion epochs in M31 from two distinct populations of globular clusters
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TN_cdi_hal_primary_oai_HAL_hal_03095182v1
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_hal_primary_oai_HAL_hal_03095182v1
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ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/s41586-019-1597-1