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  3. The early evolution of supernova remnants in a homogeneous medium - The effects of electron thermal conduction
  1. Home
  2. Publications
  3. The early evolution of supernova remnants in a homogeneous medium - The effects of electron thermal conduction

The early evolution of supernova remnants in a homogeneous medium - The effects of electron thermal conduction

Author:
  • LCL. L. Cowie
    L. L. Cowie
Publisher website
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  • 1 July 1977
    • journal article
    • Published by American Astronomical Society in The Astrophysical Journal
    • Vol. 215, 226
    • DOI:10.1086/155351
Abstract
No abstract available
Keywords
  • ENERGY TRANSFER
  • MAGNETIC FIELD
  • ELECTRON DENSITY
  • HEAT TRANSFER
  • SHOCK WAVE
  • FLUID SIMULATION
  • SHOCK WAVES
  • PLASMA
  • THERMAL CONDUCTION
  • MEAN FREE PATH
  • MAGNETIC FIELDS
  • NUMERICAL SIMULATION
  • IRON
  • LINE SPECTRA
  • FLUID MECHANICS
  • STAR EVOLUTION
  • STELLAR EVOLUTION
  • EMISSION LINE
  • HYDRODYNAMICS
  • THERMAL CONDUCTIVITY
Cited by 17 articles
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