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Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh
(Edp Sciences, 2015-01)
We investigate line formation processes in Type IIb supernovae (SNe) from 100 to 500 days post-explosion using spectral synthesis calculations. The modelling identifies the nuclear burning layers and physical mechanisms ...
Optical and near-infrared observations of sn 2011dh-the first 100 days
(SPRINGER SCIENCE, 2014)
The type IIB supernova 2011DH from a supergiant progenitor
(IOPscience, 2012)