Pulsars, Supernova Remnants and Radio Galaxies by Professor G Srinivasan

Pulsars, Supernova Remnants and Radio Galaxies by Professor G Srinivasan

International Centre for Theoretical Sciences via YouTube Direct link

Summer course 2018 - A Random walk in astro-physics

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1 of 52

Summer course 2018 - A Random walk in astro-physics

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Pulsars, Supernova Remnants and Radio Galaxies by Professor G Srinivasan

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  1. 1 Summer course 2018 - A Random walk in astro-physics
  2. 2 Pulsars, Supernova Remnants and Radio Galaxies Lecture - 05
  3. 3 The remarkable story of the Crab Nebula
  4. 4 Guest Stars
  5. 5 Guest Star of 1054 A.D.
  6. 6 Line emission & Continuum emission
  7. 7 Continuous emission is strongly polarized
  8. 8 Expanding wisps near the centre of the nebula
  9. 9 Crab Nebula is expanding with a velocity approximate 1500 km per second
  10. 10 Acceleration of the nebula!
  11. 11 Radio emission from the Crab!
  12. 12 A great prediction by Shklovskii
  13. 13 Radio emission from the Crab Nebula is very strongly linearly polarized.
  14. 14 X-Ray emission from the nebula!
  15. 15 The great puzzle!
  16. 16 The great central engine
  17. 17 An extraordinary conjecture by Pacini!
  18. 18 Properties of neutron stars
  19. 19 Oscillating charge will radiate
  20. 20 Pulsars
  21. 21 Twinkle, twinkle little star
  22. 22 A video made with a TV camera showed that Baade's star pulsed with a period of 33 ms!
  23. 23 The great prediction by Franco Pacini
  24. 24 Neutron Stars as Pulsars
  25. 25 Neutron stars are powerful dynamos!
  26. 26 Pulsar electrodynamics
  27. 27 Magnetosphere of the neutron star
  28. 28 Light Cylinder
  29. 29 The Polar Cap Model for pulsars
  30. 30 Radio radiation from pulsars
  31. 31 A hollow cone of radiation
  32. 32 Radiation from a relativistic charge
  33. 33 Coherence of the radio radiation
  34. 34 Radio Galaxies and Quasars
  35. 35 The Radio Galaxy Cygnus A
  36. 36 Origin of the radio lobes
  37. 37 Jets discovered in Cygnus A
  38. 38 One sided jets
  39. 39 NGC 6251
  40. 40 Proper time:
  41. 41 Doppler Shift
  42. 42 Doppler favoritism
  43. 43 Superluminal motion
  44. 44 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.
  45. 45 Relativistic jets
  46. 46 Energy content
  47. 47 The central engine
  48. 48 Eddington Luminosity Limit
  49. 49 Variability of Quasars
  50. 50 Supermassive Black Holes
  51. 51 Next Lecture: Compton Scattering and Celestial Gamma Ray Sources
  52. 52 Q&A

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