The Realm of Supermassive Black Holes - Lecture 13

The Realm of Supermassive Black Holes - Lecture 13

International Centre for Theoretical Sciences via YouTube Direct link

Superluminal motion

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24 of 65

Superluminal motion

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The Realm of Supermassive Black Holes - Lecture 13

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  1. 1 Date: Wed, 26 June 2019, 10:00 to
  2. 2 Neutron Stars and Black Holes Lecture -13: The Realm of the Supermassive Black Holes
  3. 3 Realm of the Supermassive Black Holes
  4. 4 The Radio Galaxy Cygnus A
  5. 5 Cliff top Interferometer
  6. 6 Intensity Interferometer
  7. 7 Hanbury-Brown & Twiss Intensity Interferometer
  8. 8 Michelson Interferometer
  9. 9 Intensity Interferometer of Hanbury-Brown
  10. 10 The Radio Galaxy Cygnus A
  11. 11 Quest for high angular resolution
  12. 12 Origin of the radio lobes
  13. 13 Jets discovered in Cygnus A
  14. 14 Very Long Baseline Interferometry
  15. 15 The Global VLBI-Array
  16. 16 CYGNUS A
  17. 17 One sided jets
  18. 18 M 87 The giant elliptical
  19. 19 NGC 6251
  20. 20 Proper time:
  21. 21 Doppler Shift
  22. 22 Doppler favoritism
  23. 23 Imagine a black hole at position A ejecting a blob in direction making an angle theta to the observer. Let the blob be moving with velocity v.
  24. 24 Superluminal motion
  25. 25 Apparent transverse velocity as a function of beta and theta
  26. 26 Superluminal Motion in the M87 Jet
  27. 27 To achieve sub-milli arc second resolution one uses intercontinental baseline interferometry.
  28. 28 Relativistic jets
  29. 29 Energy content in the radio lobes
  30. 30 Energy content
  31. 31 The central engines
  32. 32 Eddington Luminosity Limit
  33. 33 Thompson scattering cross section:
  34. 34 Variability of Quasars
  35. 35 Supermassive Black Holes
  36. 36 Accretion onto Supermassive Black Holes
  37. 37 Evidence for supermassive Black Holes
  38. 38 NGC 4258
  39. 39 Mega MASERS in NGC 4258
  40. 40 Stars orbiting the Galactic Centre Black Hole
  41. 41 Black Hole at the centre of Milky Way
  42. 42 The giant black hole at the center of M 87
  43. 43 M87 Base of Jet
  44. 44 Angular resolution required to resolve the event horizon of the central BH
  45. 45 VLBI at 1.3 mm
  46. 46 Event Horizon Telescope
  47. 47 VLBI at 1.3 mm with the EHT
  48. 48 Environment of the Black Hole
  49. 49 What does one expect to see with the EHT?
  50. 50 Motion of light near a nonrotating BH
  51. 51 What does one expect to see?
  52. 52 Comparison with simulations suggests that the torus is rotating CLOCKWISE around the spin axis of the BH
  53. 53 Summary of the conclusions
  54. 54 Has General Relativity finally been verified to a satisfactory extent?
  55. 55 S. Chandrasekhar:
  56. 56 X-Ray interferometry - in the near future - and, to a lesser extent, space based GW detectors hold out tantalizing prospects
  57. 57 Formation of supermassive black holes
  58. 58 Mergers
  59. 59 How did the original BHs form?
  60. 60 Supermassive stars
  61. 61 Stability of Matter
  62. 62 Stability of a star in General Relativity
  63. 63 Stability of a supermassive star in General Relativity
  64. 64 Next Lecture - Universe or Multiverse?!
  65. 65 Q&A

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