The tight subgiant branch of the intermediate-age star cluster NGC 411 implies a single-aged stellar population (2016)
Attributed to:
Astrophysics Research at Liverpool John Moores University: Consolidated Grant Renewal
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stw1491
Publication URI: http://dx.doi.org/10.1093/mnras/stw1491
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3