The evolution of the UV luminosity function of globular clusters 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
Funder
European Research Council
Royal Society
German Research Foundation
Emmy Noether Research Group
University of Heidelberg
Durham University
STFC
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/stz1592/28790786/stz1592.pdf
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2. Probing the role of the galactic environment in the formation of stellar clusters, using M83 as a test bench
3. On the star formation rate - brightest cluster relation: estimating the peak star formation rate in post-merger galaxies
4. Multiple Stellar Populations in Globular Clusters
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