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The young protostellar disk in IRAS16293-2422 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/10.48550/arxiv.2109.06497

Publication URI: https://arxiv.org/abs/2109.06497

Type: Other