Sheets, filaments and clumps - high resolution simulations of how the thermal instability can form molecular clouds (2018)
Attributed to:
A Programme in Astrophysical Theory and Observations at Leeds
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1812.09051
Publication URI: https://arxiv.org/abs/1812.09051
Type: Other