Abstract
The fully implicit high-order scheme has been developed for time-dependent multi-group radiative transfer coupled with implicit hydrodynamics. The application of this scheme to SN 1987A explosion shows that shortly after the shock breakout there forms a dense shell.
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Blinnikov, S.I., Nadyozhin, D.K. (1991). Modelling of the Early Light Curve of SN 1987A with the Multi-Group Time-Dependent Radiative Transfer. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_27
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DOI: https://doi.org/10.1007/978-1-4612-2988-9_27
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