Is the escape velocity in star clusters linked to extended star formation histories? Using NGC 7252: W3 as a test case (2016)

First Author: Cabrera-Ziri I
Attributed to:  Astrophysics Research at Liverpool John Moores University: Newly Appointed Academic Staff funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stv2977

Publication URI: http://dx.doi.org/10.1093/mnras/stv2977

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 1