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Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf5 May 2017: in thePSF (figure 1 middle) that result from the interferometricnature of the observations. ... Middle: Model convolved with the dirty beam and attenuated by the primary beam. -
arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf5 May 2017: By repeatingthis prescription for synthetic data we are able to test different scenarios for how the occultationsdo or do not repeat. ... We leave the development of a quantitative study of thisscenario for the future, noting that tests of such a model -
Circumstellar discs: What will be next? Quentin Kral, Cathie ...
https://people.ast.cam.ac.uk/~wyatt/kcw17.pdf13 Nov 2017: Currently efforts to test this scenario observationallyare in their infancy and over-lap with efforts to test models for photoevaporation(see below). -
MNRAS 000, 1–24 (2017) Preprint 30 March 2017 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/rwt17.pdf5 May 2017: 16) and eq. (17). For the top panels i = 10,for the middle panels m3 = 1MJ and for the bottom panels a3 = 2au. -
, DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...
https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf23 Dec 2017: These re-sults advocate for additional tests with the various proposedcircumstellar scenarios in order to resolve whether the dy-namical history of such material could produce the shapes ofthe dips. ... In the middle of SkaraBrae (on UT 2017 August 8; JD
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