Planet formation around M dwarfs via disc instability Fragmentation conditions and protoplanet properties (2020)

First Author: Mercer A

Attributed to: DiRAC 2.5y Bridging Funding - UCL funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201936954

Publication URI: http://dx.doi.org/10.1051/0004-6361/201936954

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics