The age-mass-metallicity-activity relation for solar-type stars: comparisons with asteroseismology and the NGC 188 open cluster (2016)

First Author: Lorenzo-Oliveira D
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/10.1051/0004-6361/201629233

Publication URI: http://dx.doi.org/10.1051/0004-6361/201629233

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics