H α morphologies of star clusters in 16 LEGUS galaxies: Constraints on H ii region evolution time-scales

H α morphologies of star clusters in 16 LEGUS galaxies: Constraints on H ii region evolution time-scales

The analysis of star cluster ages in tandem with the morphology of their H ii regions can provide insight into the processes that clear a cluster's natal gas, as well as the accuracy of cluster ages and dust reddening derived from Spectral Energy Distribution (SED) fitting. We classify 3757 sta...

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Bibliographic Details
Main Authors: Adamo, A. (Author), Barnes, A.T (Author), Belfiore, F. (Author), Boquien, M. (Author), Calzetti, D. (Author), Chandar, R. (Author), Della Bruna, L. (Author), Groves, B. (Author), Hannon, S. (Author), Kreckel, K. (Author), Lee, J.C (Author), Linden, S. (Author), Mobasher, B. (Author), Orozco-Duarte, R. (Author), Thilker, D. (Author), Whitmore, B.C (Author), Wofford, A. (Author)
Format: Article
Language:English
Published: Oxford University Press 2022
Subjects:
Distribution fitting
Galaxies
galaxies: ISM
Galaxies: ISM
galaxies: star clusters: general
Galaxies: star clusters: generals
H ii region
H ii regions
Hubble space telescopes
ISM: evolution
ISM:evolution
Morphology
Partially exposed
Spectral energy distribution
Star clusters
Stars
Stochastic systems
Time-scales
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