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Publications of the Astronomical Society of Australia (PASA)doi:…
https://people.ast.cam.ac.uk/~wyatt/khna21.pdf23 Nov 2021: The HD J = 2 1 line is stronger for low mass op-tically thin disks (1019 W m2) and fainter for opticallythick massive disks (1018 W m2).Since the line fluxes ... Due to the lower op-tical depth with respect to the main isotopologue, the13CO transitions -
MNRAS 000, 1–23 (2021) Preprint 1December 2021 Compiled…
https://people.ast.cam.ac.uk/~wyatt/rw21.pdf2 Dec 2021: MNRAS 000, 1–23 (2021) Preprint 1December 2021 Compiled usingMNRASLATEXstyle file v3.0. Comet fragmentation as a source of the zodiacal cloud. JessicaK.Rigley,1 MarkC.Wyatt,11Institute of Astronomy, University of Cambridge, Madingley Road, -
MNRAS 000, 1–23 (2020) Preprint 14 June 2021 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/lmwk21.pdf16 Jul 2021: MNRAS 000, 1–23 (2020) Preprint 14 June 2021 Compiled usingMNRASLATEXstyle file v3.0. High resolution ALMA and HST images of q1 Eri: an asymmetricdebris disc with an eccentric Jupiter. J. B. Lovell1, S.Marino1,2,M.C.Wyatt1,
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