A dusty origin for the correlation between protoplanetary disc accretion rates and dust masses (2020)

First Author: Sellek A
Attributed to:  Consolidated Grant Astronomy Observation and Theory 2019-2022 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa2519

Publication URI: http://dx.doi.org/10.1093/mnras/staa2519

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society

Issue: 2