The young protostellar disc in IRAS 16293-2422 B is hot and shows signatures of gravitational instability (2021)

First Author: Zamponi J
Attributed to:  A Programme of Astrophysical Theory and Observations at Leeds funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stab2657

Publication URI: http://dx.doi.org/10.1093/mnras/stab2657

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2