Can circumstellar interaction explain the strange light-curve features of Type Ib/c supernovae?

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Table 1.

Physical properties of our single-star models.

No.	M (M_⊙)	Wind type	η_wind	Z	R_p (10¹⁰ cm)	M_Ibc (M_⊙)	dM (M_⊙)	M_He (M_⊙)
S1	15	Dutch⁽¹⁾	0.8	0.02	8.93	4.28	10.72	1.81
S2	15	Dutch⁽¹⁾	0.8	0.002	4.39	4.34	10.66	1.77
S3	15	Dutch⁽¹⁾	1.0	0.02	8.45	4.36	10.64	1.83
S4	15	Reimers⁽²⁾	0.8	0.02	8.71	4.23	10.77	1.84
S5	20	Dutch⁽¹⁾	0.8	0.02	7.13	6.65	13.35	3.32
S6	20	Dutch⁽¹⁾	0.8	0.002	5.52	6.73	13.27	3.72
S7	20	Dutch⁽¹⁾	1.0	0.02	7.15	6.80	13.20	3.46
S8	20	Dutch⁽¹⁾	0.6	0.02	8.69	6.77	13.23	3.42
S9	20	Reimers⁽²⁾	0.8	0.02	7.17	6.82	13.18	3.29
S10	20	de Jager⁽³⁾	0.8	0.02	7.13	6.74	13.26	3.82
S11	20	Vink⁽⁴⁾	0.8	0.02	9.89	6.35	13.65	3.39
S12	50	Dutch⁽¹⁾	0.8	0.02	0.22	6.27	43.73	0.078
S13	50	Dutch⁽¹⁾	0.8	0.002	0.24	6.11	43.89	0.098
S14	50	de Jager⁽³⁾	0.8	0.02	0.03	6.23	43.77	0.088

Notes.

⁽¹⁾

Glebbeek et al. (2009), Nugis & Lamers (2000);

⁽²⁾

Reimers (1975),

⁽³⁾

de Jager et al. (1988),

⁽⁴⁾

Vink et al. (2001).

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