Persistent URL of this record https://hdl.handle.net/1887/3561750
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- MNRAS_514_2022_1088
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Modelling the secular evolution of protoplanetary disc dust sizes: a comparison between the viscous and magnetic wind case
- All authors
- Zagaria, F.; Rosotti, G.P.; Clarke, C.J.; Tabone, B.
- Date
- 2022
- Volume
- 514
- Issue
- 1
- Pages
- 1088 - 1106