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/10.1051/0004-6361/201526295

Publication URI: http://dx.doi.org/10.1051/0004-6361/201526295

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics