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Fig. 6


Comparisons between the cumulative NCR distributions of various SN types and stellar samples in the LMC and/or M 33. Panel a) type II-P SNe; b) type II-L; c) type IIb; d) type Ib; e) type Ic from A12; f) type Ic from K13 and g) type IIn. The stellar samples have been selected based on formal consistency according to the AD test (ten per cent probability of the distributions being the same) and similar mean NCRs. In the case of the type IIn SNe, we also include the LBVs to demonstrate the difference of these distributions.

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