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28 Oct 2013: et al., 2013, A&A 555, A11Eiroa C. et al., 2010, A&A 518, L131Figueira P. ... von Braun K. et al., 2011, ApJ 729, L26. Watson C.A.

22 Aug 2014: C. WyattInstitute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK. ... component. c 0000 RAS, MNRAS000, 000–000. Two Temperature Debris Disks: Multiple Belts?

4 Dec 2014: 3 P R O P E R T I E S O F A - S TA R D E B R I S D I S C S. ... 0P. 160. R16. 0χ. 160. nam. ety. pe(p. arse. c)(M. yr).

11 Apr 2019: Cotton1,2?, Jonathan P. Marshall3,4, Priscilla C. Frisch5,Lucyna Kedziora-Chudzer1,2, Jeremy Bailey1,2, Kimberly Bott6,7,Duncan J. ... 2010;Cotton et al. 2016b,c; Frisch et al. 2016; Cotton et al.

29 Apr 2016: Filter HD T/C λeff q u p d p/d θ[nm] [ppm] [ppm] [ppm] [pc] [ppm/pc] []. g′ 2262 Target 464.2 4.7 5.7 37.4 ... Sub-micron (0.1µm) dust grains are predicted to have. 10 J. P.

8 Jan 2019: Matrà7. and M. C. Wyatt11Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK2Max Planck Institute for Astronomy, Königstuhl 17, 69117 Heidelberg, Germany3Astrophysikalisches Institut und Universitätssternwarte

14 Nov 2013: of Fomalhaut b, though itnow appears to apply to a hypothetical Fomalhaut c(Chiang et al. ... 2009).The suggestion that the entire HR 8799 system may be. coplanar is consistent with the results of Watson et al.(2011) and Greaves et al.

17 Dec 2014: Five steps in the evolution from protoplanetary to debrisdisk. M. C. ... M. C. Wyatt. O. Panić. G. M. Kennedy. L. Matrà. Institute of Astronomy, University of Cambridge, MadingleyRoad, Cambridge CB3 0HA, UK.

19 Feb 2018: 3 D I S C I N C I D E N C E A R O U N D F, G , A N D KT Y P E S TA ... 4(c), is 28 per cent,the same as that given in Table 2.

31 Jul 2018: S. Marino,1?, J. Carpenter,2 M. C. Wyatt1, M. Booth3, S. Casassus4,5, V. ... P] 3. Jul. 201. 8. 2 S. Marino et al. than 10 au it has only been possible to detect a few gas gi-ants, mainly through direct imaging 1 (Marois