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2-3, D-07745 Jena, GermanyDraft version February 14, 2023Typeset…
https://people.ast.cam.ac.uk/~wyatt/mbpw22.pdf22 Mar 2024: Stapelfeldt ,22. Jordan M. Stone ,23 Jason J. Wang ,24, 25 Olivier Absil ,26 William O. ... MIRI Channel 4, Medium B 20.69 - 24.44 FULL FASTR1 1,680 – 1,770 1576.22. -
DRAFT VERSION JULY 17, 2023Typeset using LATEX twocolumn style ...
https://people.ast.cam.ac.uk/~wyatt/srw23.pdf22 Mar 2024: Equations (24)–(27). 4 A. A. SEFILIAN, R. R. RAFIKOV, & M. -
MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/hwd22.pdf22 Mar 2024: MNRAS 000, 1–14 (2022) Preprint 18 January 2023 Compiled usingMNRASLATEXstyle file v3.0. Has the dust clump in the debris disk of Beta Pictoris moved? Y.Han,1 M.C.Wyatt,1 W.R. F.Dent,21Institute of Astronomy, University of Cambridge, Madingley Road -
MNRAS 000, 1–17 (2033) Preprint 19 June 2023 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/tmbh23.pdf22 Mar 2024: M = H(q)𝑇 N1H(q), (23). j = H𝑇 N1V. (24). Finally, I𝑠 = 𝝁 is used as the inferred brightness. ... 2). (27). This change to H(q) is used in Equations 21–24 or when comput-ing the model visibilities (Equation 18), with the code -
Inner edges of planetesimal belts: collisionally eroded or truncated?
https://people.ast.cam.ac.uk/~wyatt/immb23.pdf20 Feb 2024: 33 obs D 0. 06 max. (24). max = 2. 7 10 27 M 3. ... 67 c D 0. 65 obs. (26) hen comparing equation ( 24 ) with the numerical model fromarino et al. (
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