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  2. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_10.pdf
    22 Oct 2017: 2013, ApJ, 775, L7, summary Smartt 2015, PASA, 32, 16. • Key test of stellar evolution models for short-lived high-mass stars would be to identify exact nature of star when ... Star of the Week – direct test of the evolutionary models for high mass
  3. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 Nov 2017: Structure & Evolution of Stars 13. VY Canis Majoris• The Lithium-test for classification as star or brown dwarf works for stars on or close to the main sequence – relatively strong neutral ... Can also use Lithium test to discriminate between
  4. publications

    https://people.ast.cam.ac.uk/~mjr/publications/
    18 Oct 2017: Field and D.W. Sciama). On the V/V. m. Test applied to Quasi-Stellar Radio Sources. ... W. Brinkmann (MPI Publications). Tests for the minihalo model of the Lyman alpha forest.
  5. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_19.pdf
    16 Nov 2017: sequence that gives rise to the recently created white dwarfs – can perform direct test of stellar evolution theory• Evolution of stars from horizontal branch to white dwarf is almost instantaneous relative
  6. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_21.pdf
    17 Nov 2017: sunns. LLT. RRTRL. • Rich variety of phenomena now known. Powerful tests of General Relativity using close binary pulsars now possible – multiple Nobel Prizes! •
  7. arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf
    5 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
  8. Draft v7.0Preprint typeset using LATEX style AASTeX6 v. 1.0 ...

    https://people.ast.cam.ac.uk/~wyatt/mrdk17.pdf
    11 Sep 2017: ABSTRACT. To test alternative hypotheses for the behavior of KIC 8462852, we obtained measurements of the star. ... they should be negligible for the Spitzer measurements.). To test for such effects, we turned to the photometry of.
  9. Circumstellar discs: What will be next? Quentin Kral, Cathie ...

    https://people.ast.cam.ac.uk/~wyatt/kcw17.pdf
    13 Nov 2017: Currently efforts to test this scenario observationallyare in their infancy and over-lap with efforts to test models for photoevaporation(see below).
  10. Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf
    5 May 2017: Preliminary tests showed good fits in two re-gions of parameter space, which we, therefore, split into twoMCMC runs: run A, which is constrained to be a narrowbelt (with Rin > 57 ... 2011). As in MacGregor et al. (2015), we also con-sider a Gaussian
  11. arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf
    26 Sep 2017: young FG-type stars. By applying a Fisher’s exact test. to compare the occurrence of CO-bearing disks in the.
  12. arX iv:1 702. 0512 3v1 [as tro- ph.E P] ...

    https://people.ast.cam.ac.uk/~wyatt/bfwv17.pdf
    5 May 2017: Future observations sensitive tofaint infrared excesses or the presence of gas, can test the scenarios presented here,thereby better constraining the nature of the material fuelling accretion in pollutedwhite dwarfs.
  13. Preprint typeset using LATEX style emulateapj v. 01/23/15 DETECTION…

    https://people.ast.cam.ac.uk/~wyatt/mmkwk17.pdf
    18 May 2017: 3.2. Spectral spatial filter: SNR boost and kinematics. In order to test the robustness and improve the signif-icance of the detection, we make the further assumptionthat the CO gas ... Finally, we test for any indication of azimuthal asym-metry in the
  14. , DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...

    https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf
    23 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.
  15. Mon. Not. R. Astron. Soc. 000, 1–27 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmwk17.pdf
    5 May 2017: ABSTRACTThis paper uses observations of dusty debris discs, including a growing number ofgas detections in these systems, to test our understanding of the origin and evolutionof this gaseous component. ... 2015), and motivating the need for line ratiosto
  16. MNRAS 000, 1–24 (2017) Preprint 30 March 2017 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rwt17.pdf
    5 May 2017: MNRAS 000, 1–24 (2017) Preprint 30 March 2017 Compiled using MNRAS LATEX style file v3.0. Transit Probabilities in Secularly Evolving PlanetarySystems. Matthew J. Read1,? Mark C. Wyatt1 and Amaury H. M. J. Triaud11Institute of Astronomy,

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