Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/39881
Title: Star clusters as building blocks for dSph galaxy formation
Authors: Assmann, P.
Fellhauer, M.
Wilkinson, Mark I.
First Published: 1-Jan-2010
Publisher: Cambridge University Press (CUP) for International Astronomical Union (IAU)
Citation: Proceedings of the International Astronomical Union, 2009, 5 (S266 Star clusters: basic galactic building blocks throughout time and space), pp. 353-356
Abstract: We study numerically the formation of dSph galaxies. Intense starbursts, e.g., in gas-rich environments, typically produce a few to a few hundred young star clusters within a region of just a few hundred pc. The dynamical evolution of these star clusters may explain the formation of the luminous component of dwarf spheroidal (dSph) galaxies. Here, we perform a numerical experiment to show that the evolution of star cluster complexes in dark-matter haloes can explain the formation of the luminous components of dSph galaxies. © International Astronomical Union 2010.
DOI Link: 10.1017/S174392130999127X
ISSN: 1743-9213
eISSN: 1743-9221
Links: https://www.cambridge.org/core/journals/proceedings-of-the-international-astronomical-union/article/star-clusters-as-building-blocks-for-dsph-galaxy-formation/F43F904D72B8758E9977F272FA1AC1A6
http://hdl.handle.net/2381/39881
Version: Post-print
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2010, International Astronomical Union. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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