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11 - 20 of 38 search results for TALK:PC53 20 |u:people.ast.cam.ac.uk where 0 match all words and 38 match some words.

  1. Results that match 1 of 2 words

  2. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_13.pdf
    2 Nov 2017: Mass estimate 18-25 solar masses (from models). Structure & Evolution of Stars 20. ... Slide Number 18. Slide Number 19. Slide Number 20. Slide Number 21.

  3. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_02.pdf
    9 Oct 2017: Wien’s Displacement Law. T (K) λ (μm) Source. 20 145 Molecular cloud293 9.9 Room temperature. ... Slide Number 20. Slide Number 21. Slide Number 22. Wien’s Displacement Law.

  4. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_17.pdf
    10 Nov 2017: Energy generation from the twin shells is enormous. Structure & Evolution of Stars 20. ... Slides 6, 8, 10, 14, 15, 20 and 22 from F Shu, University Science Books.

  5. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_18.pdf
    10 Nov 2017: Structure & Evolution of Stars 19. Structure & Evolution of Stars 20. ... Slide Number 19. Slide Number 20. Slide Number 21. Slide Number 22.

  6. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_23.pdf
    24 Nov 2017: For small R, neutron star with 𝑅𝑅 104m and 𝑀𝑀 1.5MSun then 20% of rest-mass (𝑚𝑚𝑐𝑐2) liberated as material reaches neutron star surface, cf energy from nuclear fusion, 1% ... rdr. PdP. rPr. GmdmdP. 4. 4. 4. 4. 20. 44. =. ===. =. =.

  7. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_09.pdf
    20 Oct 2017: Structure & Evolution of Stars 20. Lecture 9: Summary• Opacity – have looked at the dependence on density,. ... Slide Number 18. Slide Number 19. Slide Number 20. Picture Credits.

  8. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_15.pdf
    6 Nov 2017: at low T and polytropic index for fully convective star is n=1.5 and A=20 – an almost vertical track in the HR-diagram• As the mass of the protostar ... Slide Number 18. Slide Number 19. Slide Number 20. Slide Number 21.

  9. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_16.pdf
    10 Nov 2017: Structure & Evolution of Stars 20. Absorption line profiles of transitions in neutral Fe and Ti towards the star and at distances further out across the nebulaNote the sharp features present in ... Slides 3 and 17 Ostlie and Carroll• Slide 7 Digital

  10. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_14.pdf
    6 Nov 2017: Structure & Evolution of Stars 20. Solving the Equations of Stellar Structure• One class of special cases arises when the pressure depends only on the density so that there is no ... Slide Number 18. Slide Number 19. Slide Number 20. Slide Number 21.

  11. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_19.pdf
    16 Nov 2017: would be reassuring. Structure & Evolution of Stars 20. Structure & Evolution of Stars 21. ... Compare to the ratio of the populations in the “Blue Clump” compared to the rest of the population on the Horizontal Branch –only 20% of the He-rich bMS

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