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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_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_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_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_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_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_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_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_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_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_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_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_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). •
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