Preprint
Observational constraints on star cluster formation theory - I. The mass-radius relation
Abstract
Stars form predominantly in groups usually denoted as clusters or
associations. The observed stellar groups display a broad spectrum of masses,
Authors
Pfalzner S; Kirk H; Sills A; Urquhart JS; Kauffmann J; Kuhn MA; Bhandare A; Menten KM
Publication date
December 1, 2015
DOI
10.48550/arxiv.1512.00334
Preprint server
arXiv