The globular cluster system mass–halo mass relation in the E-MOSAICS simulations
Author:
Affiliation:
1. Astrophysics Research Institute, Liverpool John Moores University, 146 Brownlow Hill, Liverpool L3 5RF, UK
2. Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstrasse 12-14, D-69120 Heidelberg, Germany
Abstract
Funder
Royal Society
H2020 European Research Council
Deutsche Forschungsgemeinschaft
Universität Heidelberg
British Interplanetary Society
Science and Technology Facilities Council
Durham University
Liverpool John Moores University
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/staa2453/33664200/staa2453.pdf
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4. UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
5. Globular Clusters in Dense Clusters of Galaxies
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