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

First Author: Mercer A
Attributed to:  Consolidated Solar and Astrophysics Research at UCLan funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2001.10062

Publication URI: https://arxiv.org/abs/2001.10062

Type: Other