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1 - 32 of 32 search results for TALK:Vb20 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_24.pdf
    24 Nov 2017: Structure and Evolution of Stars 1. Structure and Evolution of StarsLecture 24: Extreme and some Fun Stars. •

  3. Martin Rees: Short Articles & Miscellaneous Journalism

    https://people.ast.cam.ac.uk/~mjr/shortpop.html
    18 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.

  4. MNRAS 000, 1–24 (2017) Preprint 30 March 2017 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/rwt17.pdf
    5 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.

  5. Martin Rees: Chapters in books and longer popular articles

    https://people.ast.cam.ac.uk/~mjr/longpop.html
    18 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).

  6. 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.

  7. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_03.pdf
    9 Oct 2017: Structure & Evolution of Stars 23. Structure & Evolution of Stars 24. ... Slide Number 23. Slide Number 24. Slide Number 25. Slide Number 26.

  8. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_13.pdf
    2 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.

  9. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_15.pdf
    6 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

  10. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_18.pdf
    10 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.

  11. 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.

  12. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_20.pdf
    16 Nov 2017: Structure & Evolution of Stars 23. Structure & Evolution of Stars 24. ... Slide Number 22. Slide Number 23. Slide Number 24. Slide Number 25.

  13. 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.

  14. 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.

  15. 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.

  16. 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

  17. 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. •

  18. 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.

  19. 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.

  20. 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). •

  21. 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).

  22. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_04.pdf
    13 Oct 2017: Structure & Evolution of Stars 24. Spectroscopic Binaries. 231. 32. 21.

  23. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_02.pdf
    9 Oct 2017: Wien’s Law is extraordinarily useful and worth remembering. Structure & Evolution of Stars 24.

  24. PowerPoint Presentation

    https://people.ast.cam.ac.uk/~phewett/SandES2017/Lec2017_21.pdf
    17 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.

  25. Accepted to ApJ: April 6, 2017Preprint typeset using LATEX ...

    https://people.ast.cam.ac.uk/~wyatt/mmkwp17.pdf
    18 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.

  26. MNRAS 000, 1–16 (2017) Preprint 21 November 2017 Compiled ...

    https://people.ast.cam.ac.uk/~wyatt/xrvv17.pdf
    21 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.

  27. Mon. Not. R. Astron. Soc. 000, 1–27 (2002) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/kmwk17.pdf
    5 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

  28. Mon. Not. R. Astron. Soc. 000, 000–000 (2017) Printed ...

    https://people.ast.cam.ac.uk/~wyatt/bdjl17.pdf
    5 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

  29. arX iv:1 709. 0841 4v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/mcka17.pdf
    26 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.

  30. Draft v7.0Preprint typeset using LATEX style AASTeX6 v. 1.0 ...

    https://people.ast.cam.ac.uk/~wyatt/mrdk17.pdf
    11 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.

  31. , DRAFT VERSION DECEMBER 23, 2017Typeset using LATEX twocolumn ...

    https://people.ast.cam.ac.uk/~wyatt/baaa18.pdf
    23 Dec 2017: BURDANOV,8 B. CALE,24 MIGUEL AZNAR CARBO,25 R. CASTILLO GARCÍA,26, 4, 27.

  32. Circumstellar discs: What will be next? Quentin Kral, Cathie ...

    https://people.ast.cam.ac.uk/~wyatt/kcw17.pdf
    13 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

  33. arX iv:1 701. 0656 8v1 [as tro- ph.S R] ...

    https://people.ast.cam.ac.uk/~wyatt/kkpr17.pdf
    5 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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