Modelling circumbinary protoplanetary disks: I. Fluid simulations of the Kepler-16 and 34 systems (2015)

First Author: Lines S

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/10.48550/arxiv.1507.06998

Publication URI: https://arxiv.org/abs/1507.06998

Type: Other