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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/10.48550/arxiv.2008.07530

Publication URI: https://arxiv.org/abs/2008.07530

Type: Other