5 Interacting supernovae and the influence on spectra and light curves

5.1 Introduction 5.2 Interaction regimes and optical signatures

 5.2.1. Rarefied CSM: absorption signatures
 5.2.2  Dense CSM: emission lines and continuum
 5.2.3  Cool dense shell fragmentation and CSM clumpiness

5.3 Supernovae powered by collision of massive shells

  5.3.1 Multiple shell ejection by massive stars
  5.3.2 Interaction with radiation trapping effects
  5.3.3 X-ray emission weakness from luminous interactors

5.4 Conclusion

public/blinnikov-plan.txt · Last modified: 2015/10/21 10:10 by Stephen Smartt

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