Efficiency of tidal dissipation in slowly rotating fully convective stars or planets (2020)
Attributed to:
DiRAC-2.5 - the pathway to DiRAC Phase 3
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2007.13392
Publication URI: https://arxiv.org/abs/2007.13392
Type: Other