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

First Author: Facchini S
Attributed to:  Astronomy Observation and Theory Consolidated Grant 2016-2019 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.17863/cam.40446

Publication URI: https://www.repository.cam.ac.uk/handle/1810/293292

Type: Journal Article/Review