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11 - 20 of 32 search results for katalk:PC53 24 / |u:people.ast.cam.ac.uk where 0 match all words and 32 match some words.

  1. Results that match 1 of 2 words

  2. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 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.

  3. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_10.pdf
    22 Oct 2017: Structure & Evolution of Stars 23. Structure & Evolution of Stars 24. ... Slide Number 21. Slide Number 22. Slide Number 23. Slide Number 24.

  4. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_17.pdf
    10 Nov 2017: Structure & Evolution of Stars 24. Structure & Evolution of Stars 25. ... Slide Number 21. Slide Number 22. Slide Number 23. Slide Number 24.

  5. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_08.pdf
    24 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.

  6. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_22.pdf
    17 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

  7. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_19.pdf
    16 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. •

  8. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_23.pdf
    24 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.

  9. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_11.pdf
    24 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.

  10. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_05.pdf
    12 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). •

  11. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_09.pdf
    20 Oct 2017: is:. ρεπ 24 rdrdL. =. providing 3rd equation of stellar structure (already have Hydrostatic Equilibrium, and mass conservation from Lecture 6).

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