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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_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_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_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_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_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_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_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_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.
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