Theoretical predictions for IMF diagnostics in UV spectroscopy of star clusters (2018)
Attributed to:
Durham DiRAC-2 petascale facility
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1807.11524
Publication URI: https://arxiv.org/abs/1807.11524
Type: Other