The prevalence of star formation as a function of Galactocentric radius (2016)

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stw1870

Publication URI: http://dx.doi.org/10.1093/mnras/stw1870

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 3