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Heart of darkness: dust obscuration of the central stellar component in globular clusters younger than ~100 Myr in multiple stellar population models (2015)

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnrasl/slu203

Publication URI: http://dx.doi.org/10.1093/mnrasl/slu203

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society: Letters

Issue: 1

ISSN: 0035-8711