[C]

@article{deQuincey2000C,
  title={[C]},
  author={Thomas de Quincey},
  journal={The Works of Thomas De Quincey, Vol. 1: Writings, 1799–1820},
  year={2000}
}
  • Thomas de Quincey
  • Published 1 January 2000
  • Physics
  • The Works of Thomas De Quincey, Vol. 1: Writings, 1799–1820
In supernova (SN) spectroscopy relatively little attention has been given to the properties of optically thick spectral lines in epochs following the photosphere’s recession. Most treatments and analyses of post-photospheric optical spectra of SNe assume that forbidden-line emission comprises most if not all spectral features. However, evidence exists that suggests that some spectra exhibit line profiles formed via optically thick resonance-scattering even months or years after the SN explosion… 
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VILNIUS UNIVERSITY CENTER FOR PHYSICAL SCIENCES AND TECHNOLOGY
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