What are protoclusters? – Defining high-redshift galaxy clusters and protoclusters
We explore the structures of protoclusters and their relationship with high-redshift clusters using the Millennium Simulation combined with a semi-analytic model. We find that protoclusters are very extended, with 90 per cent of their mass spread across∼35 h−1 Mpc commoving at z =2 (∼30 arcmin). The...
| Main Authors: | , , |
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| Format: | Article |
| Published: |
Oxford University Press
2015
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| Subjects: | |
| Online Access: | https://eprints.nottingham.ac.uk/34868/ |