Mass Determinations of Star Clusters

Georges Meylan

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arXiv · astro-ph/0107063

Mass Determinations of Star Clusters

Georges Meylan

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Abstract

Mass determinations are difficult to obtain and still frequently characterised by deceptively large uncertainties. We review below the various mass estimators used for star clusters of all ages and luminosities. We highlight a few recent results related to (i) very massive old star clusters, (ii) the differences and similarities between star clusters and cores of dwarf elliptical galaxies, and (iii) the possible strong biases on mass determination induced by tidal effects.

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Georges Meylan. 2001-07-03. Mass Determinations of Star Clusters. https://arxiv.org/abs/astro-ph/0107063

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