High gas-to-dust size ratio indicating efficient radial drift in the mm-faint CX Tauri disk (2019)

First Author: Facchini S
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/10.1051/0004-6361/201935496

Publication URI: http://dx.doi.org/10.1051/0004-6361/201935496

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics