Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh

A. Jerkstrand; M. Ergon; S. J. Smartt; C. Fransson; J. Sollerman; S. Taubenberger; M. Bersten; J. Spyromilio

doi:10.1051/0004-6361/201423983

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Volume 573 (January 2015)

A&A, 573 (2015) A12

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Fig. 8

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SN 2008ax (dereddened and redshift corrected) at 280 days (red), and model 13G at 300 days (black) (rescaled with exp⁽ + 2 × 20 / 111.4⁾ to compensate for the different epoch and with a factor of 1.33 to compensate for the higher ⁵⁶Ni mass).

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