Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/37359
Title: Simulating feedback from nuclear clusters: the impact of multiple sources
Authors: Bourne, Martin A.
Power, C.
First Published: 22-Nov-2015
Publisher: Oxford University Press (OUP), Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society (February 11, 2016) 456 (1): L20-L24.
Abstract: Nuclear star clusters (NCs) are found to exist in the centres of many galaxies and appear to follow scaling relations similar to those of supermassive black holes. Previous analytical work has suggested that such relations are a consequence of feedback-regulated growth. We explore this idea using high-resolution hydrodynamical simulations, focusing on the validity of the simplifying assumptions made in analytical models. In particular, we investigate feedback emanating from multiple stellar sources rather than from a single source, as is usually assumed, and show that collisions between shells of gas swept up by feedback leads to momentum cancellation and the formation of high-density clumps and filaments. This high-density material is resistant both to expulsion from the galaxy potential and to disruption by feedback; if it falls back on to the NC, we expect the gas to be available for further star formation or for feeding a central black hole. We also note that our results may have implications for the evolution of globular clusters and stellar clusters in high-redshift dark matter haloes.
DOI Link: 10.1093/mnrasl/slv162
ISSN: 0035-8711
eISSN: 1365-2966
Links: http://mnrasl.oxfordjournals.org/content/456/1/L20
http://hdl.handle.net/2381/37359
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: © 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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