Spatial Segregation of Massive Clusters in Dwarf Galaxies

Elmegreen, Bruce G. and Adamo, A. and Boquien, M. and Bournaud, F. and Calzetti, D. and Cook, D. O. and Dale, D. A. and Duc, P.-A. and Elmegreen, D. M. and Fensch, J. and Grasha, K. and Kim, Hwi and Kahre, L. and Messa, M. and Ryon, J. E. and Sabbi, E. and Smith, L. J. (2020) Spatial Segregation of Massive Clusters in Dwarf Galaxies. The Astrophysical Journal, 888 (2). L27. ISSN 2041-8213

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Abstract

The relative average minimum projected separations of star clusters in the Legacy ExtraGalactic UV Survey (LEGUS) and in tidal dwarfs around the interacting galaxy NGC 5291 are determined as a function of cluster mass to look for cluster–cluster mass segregation. Class 2 and 3 LEGUS clusters, which have a more irregular internal structure than the compact and symmetric class 1 clusters, are found to be mass-segregated in low-mass galaxies, which means that the more massive clusters are systematically bunched together compared to the lower-mass clusters. This mass segregation is not present in high-mass galaxies or class 1 clusters. We consider possible causes for this segregation, including differences in cluster formation and scattering in the shallow gravitational potentials of low-mass galaxies.

Item Type: Article
Subjects: ArticleGate > Physics and Astronomy
Depositing User: Managing Editor
Date Deposited: 26 May 2023 08:18
Last Modified: 05 Jun 2024 10:36
URI: http://ebooks.pubstmlibrary.com/id/eprint/2878

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