Astr 501 | Lecture 35 | Fall 2018
Astronomy 501
Lecture 35, December 3 Fall 2018

Lecture Notes: pdf file

From last time: M87 Counterjet

Cosmic Rays

Basic Properties

Synchrotron Radiation

Relativistic Motion in a Uniform Magnetic Field

  • gyrofrequency
  • gyroradius
  • implications for ordinary cosmic rays and those with high and for ultra-high energies

Synchrotron Emission

  • emitted power
  • emitted spectrum

Synchrotron Self-Absorption

Awesome Example: Supernova Remnants

Awesome Example: Radio Galaxies

Radio continuum sky at 408 MHz:  synchrotron from cosmic-ray electrons

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