On the time evolution of the $M_{\rm d} - M_\star$ and $\dot M - M_\star$ correlations for protoplanetary discs: the viscous timescale increases with stellar mass (2022)
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.2206.04136
Publication URI: https://arxiv.org/abs/2206.04136
Type: Other