Efficiency of tidal dissipation in slowly rotating fully convective stars or planets (2020)
Attributed to:
DiRAC 2.5 Operations 2017-2020
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa2239
Publication URI: http://dx.doi.org/10.1093/mnras/staa2239
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 4