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PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_04.pdf13 Oct 2017: Structure & Evolution of Stars 24. Spectroscopic Binaries. 231. 32. 21. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_21.pdf17 Nov 2017: Structure & Evolution of Stars 24. Distance:117pc12Proper-Motion: 0.3 arcsec per yearVelocity 185km/sAge: 500000yr. ... Slide Number 21. Slide Number 22. Slide Number 23. Slide Number 24. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_02.pdf9 Oct 2017: Wien’s Law is extraordinarily useful and worth remembering. Structure & Evolution of Stars 24. -
Accepted to ApJ: April 6, 2017Preprint typeset using LATEX ...
https://people.ast.cam.ac.uk/~wyatt/mmkwp17.pdf18 May 2017: The total belt flux density determined for the best-fit model is 24.7 0.1 mJy (with an additional 10% uncertaintyfrom flux calibration), consistent with previous flux measurements at slightly ... Foreman-Mackey, D. 2016, The Journal of Open Source. -
MNRAS 000, 1–16 (2017) Preprint 21 November 2017 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/xrvv17.pdf21 Nov 2017: L. McClain15,22, P. Muirhead13, E. Palle23,24, P. A. Panka12,. J. Provencal25, S. ... 0.16 0.18 0.20 0.22 0.24 0.26 0.28MJD(-57476). 0.0. 0.5. 1.0. 1.5. -
Mon. Not. R. Astron. Soc. 000, 1–27 (2002) Printed ...
https://people.ast.cam.ac.uk/~wyatt/kmwk17.pdf5 May 2017: 4 104 100 0.27 1.1 103 40η Tel3 CII 22 48.2 - 24 1.3 102 7.6 104 23HD 219974 CO 14.4 71.9 6 102 60 ... 3 103 1.9 103 10HD 1318357 CO 9.2 122 6 102 50 0.47 1.5 103 16HD 1388136 CO 24.5 150.8 7.4 104 100 -
Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed ...
https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf5 May 2017: In addition to the main belt seen at long wavelengths,the 24-160 µm spectral energy distribution (SED) fromSpitzer suggests a warmer ring at 20 AU and possibly an-other at -
arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf26 Sep 2017: HD 138813 A0V 150.8 24.5 US (7) 10 (4) 194/94 9.0 104(2) 1.2 101(3) Y 1.41 0.08(5) 7.5 104. -
Draft v7.0Preprint typeset using LATEX style AASTeX6 v. 1.0 ...
https://people.ast.cam.ac.uk/~wyatt/mrdk17.pdf11 Sep 2017: KIC 8462852 20 06 15.46 44 27 24.6 11.86 0.54 0.40. ... Star 2 20 06 01.24 44 29 32.4 12.42 0.79 0.51. -
, DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...
https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf23 Dec 2017: BURDANOV,8 B. CALE,24 MIGUEL AZNAR CARBO,25 R. CASTILLO GARCÍA,26, 4, 27. -
Circumstellar discs: What will be next? Quentin Kral, Cathie ...
https://people.ast.cam.ac.uk/~wyatt/kcw17.pdf13 Nov 2017: Circumstellar discs: What will be next? Quentin Kral, Cathie Clarke and Mark Wyatt. Abstract This prospective chapter gives our view on the evolution of the study ofcircumstellar discs within the next 20 years from both observational and -
arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...
https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf5 May 2017: Two other classes are: those occulted by circumstellar material beyond &10au, suchas AA Tau and V409 Tau which show &year-long dimming events [23,24], and systems such as ǫ Aur,
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