Explaining the variability of WD 1145+017 with simulations of asteroid tidal disruption (2017)

First Author: Veras D
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