Resolved photometry of extragalactic young massive star clusters

Abstract

Aims. We present colour–magnitude diagrams (CMDs) of young massive star clusters in several galaxies located well beyond the Local Group. The richness of these clusters allows us to obtain large samples of post-main sequence stars and test how well the observed CMDs are reproduced by canonical stellar isochrones. Methods. We use imaging of seven clusters in the galaxies NGC 131

Similar works

Full text

thumbnail-image

EDP Sciences OAI-PMH repository (1.2.0)

redirect
Last time updated on 10/04/2020

This paper was published in EDP Sciences OAI-PMH repository (1.2.0).

Having an issue?

Is data on this page outdated, violates copyrights or anything else? Report the problem now and we will take corresponding actions after reviewing your request.