Abstract
Young star clusters with masses well in excess of 105 M⊙ have been observed not only in merging galaxies and large-scale starbursts, but also in fairly normal, undisturbed spiral and irregular galaxies. Here, we present virial mass estimates for a sample of 7 such clusters and show that the derived mass-to-light ratios are consistent with “normal” Kroupa-type stellar mass distributions.
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Larsen, S.S., Brodie, J.P., Hunter, D.A., Richtler, T. (2005). Young Massive Clusters in Non-Interacting Galaxies. In: De Grijs, R., González Delgado, R.M. (eds) Starbursts. Astrophysics and Space Science Library, vol 329. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3539-X_38
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DOI: https://doi.org/10.1007/1-4020-3539-X_38
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-3538-8
Online ISBN: 978-1-4020-3539-5
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