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PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_24.pdf24 Nov 2017: Structure and Evolution of Stars 1. Structure and Evolution of StarsLecture 24: Extreme and some Fun Stars. • -
Martin Rees: Short Articles & Miscellaneous Journalism
https://people.ast.cam.ac.uk/~mjr/shortpop.html18 Oct 2017: Bull. Atomic Scientists, Vol 25, No. 8 p. 24, October 1989 (with B. ... Let invention take flight as it did 300 years ago. Times, 24 May 2014. -
MNRAS 000, 1–24 (2017) Preprint 30 March 2017 Compiled ...
https://people.ast.cam.ac.uk/~wyatt/rwt17.pdf5 May 2017: MNRAS 000, 1–24 (2017). 6 M. J. Read et al. Figure 4. ... 2.3. MNRAS 000, 1–24 (2017). 12 M. J. Read et al. -
Martin Rees: Chapters in books and longer popular articles
https://people.ast.cam.ac.uk/~mjr/longpop.html18 Oct 2017: Some millennial thoughts on cosmology. Interdisciplinary Science Reviews 24, 261-268 (1999). ... Field Guide to the Invisible Universe. Discover 24, No. 12, pp 42-47 (with P Natarajan). -
publications
https://people.ast.cam.ac.uk/~mjr/publications/18 Oct 2017: Black Holes. Observatory 24, 168 (1974). A Twin-Exhaust' Model for Double Radio Sources. ... Ann. Rev. Astr. AstroPhys. 24, 471 (1984). The constants of Physics' book published by Royal Society 1983, co-editor with W.H. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_03.pdf9 Oct 2017: Structure & Evolution of Stars 23. Structure & Evolution of Stars 24. ... Slide Number 23. Slide Number 24. Slide Number 25. Slide Number 26. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_13.pdf2 Nov 2017: Structure & Evolution of Stars 24. Picture Credits. • Slide 6 Phillips, Wiley• Slides 15 and 16 Astronomical Journal• Slides 18-24 Luhmann et al. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_15.pdf6 Nov 2017: Structure & Evolution of Stars 24. • The derivation of the behaviour in the L-T plane has made the most extreme assumptions and the Hayashi Tracks for a given Mand represent the ... Structure & Evolution of Stars 26. Picture Credits. • Slide 6 -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_18.pdf10 Nov 2017: Structure & Evolution of Stars 24. Fuel Source Timescale T(109K) ρ(kg m-3). ... of table on Slide 24 from Phillips. Slide Number 1. Slide Number 2. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf10 Nov 2017: V=7.95B-V=2.24. Spectral Type: M4IITeff3000K. Significant reddening – star is cocooned. Structure & Evolution of Stars 8. ... Slides 3 and 17 Ostlie and Carroll• Slide 7 Digital Sky Survey, STScI• Slides 18, 19, 20, 21, 24 and 25. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_20.pdf16 Nov 2017: Structure & Evolution of Stars 23. Structure & Evolution of Stars 24. ... Slide Number 22. Slide Number 23. Slide Number 24. Slide Number 25. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_10.pdf22 Oct 2017: Structure & Evolution of Stars 23. Structure & Evolution of Stars 24. ... Slide Number 21. Slide Number 22. Slide Number 23. Slide Number 24. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_17.pdf10 Nov 2017: Structure & Evolution of Stars 24. Structure & Evolution of Stars 25. ... Slide Number 21. Slide Number 22. Slide Number 23. Slide Number 24. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_08.pdf24 Oct 2017: Structure & Evolution of Stars 24. Picture Credits. • Slide 17 from Green and Jones, CUP• Slides 16 Ostlie and Carroll• Slide 9 Phillips, Wiley• Slide 18 Tayler “Sun as a Star”, CUP. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_22.pdf17 Nov 2017: 24. Initial candidate list from photometry or objective-prism spectra Then follow-up promising looking candidates with moderate-resolution spectra to identify candidates with [Fe/H]<-3 (or thereabouts) Finally, obtain ... Slide Number 24. Need accurate -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_19.pdf16 Nov 2017: White Dwarfs: Gravitational Redshift. 24. 2. 2. 2. 2/1. 2. 100.3z. ... Structure & Evolution of Stars 23. Globular Cluster Omega Centauri. Structure & Evolution of Stars 24. • -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_23.pdf24 Nov 2017: ρεπ 24 rdrdL. =• If shell is in thermal equilibrium, then the energy produced within the shell equals the energy flow out of the shell. • ... Slide Number 21. Slide Number 22. Slide Number 23. Slide Number 24. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_11.pdf24 Oct 2017: 2814. 42. 42. 2412. 168. 168. n. Structure & Evolution of Stars 24. ... Slide Number 23. Slide Number 24. Slide Number 25. Lecture 11: Summary. -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_05.pdf12 Oct 2017: Structure & Evolution of Stars 24. Thermal Timescale. • Suppose that the energy source of the Sun is due only to the energy available from gravitational contraction (from infinity). • -
PowerPoint Presentation
https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_09.pdf20 Oct 2017: is:. ρεπ 24 rdrdL. =. providing 3rd equation of stellar structure (already have Hydrostatic Equilibrium, and mass conservation from Lecture 6). -
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. -
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 -
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, 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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