Explaining the variability of WD 1145+017 with simulations of asteroid tidal disruption (2017)
Attributed to:
Physical constraints on the likelihood of accreting a non-chondritic Earth
funded by
NERC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stw2748
Publication URI: http://dx.doi.org/10.1093/mnras/stw2748
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 1