The relative efficiencies of bars and clumps in driving disc stars to retrograde motion (2021)
Attributed to:
Astronomy Consolidated Grant at UCLAN
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2103.10506
Publication URI: https://arxiv.org/abs/2103.10506
Type: Other