Spectral signatures of H-rich material stripped from a non-degenerate companion by a Type Ia supernova

Open Access

Table A.1

Coefficients of the polynomial fits to the correlation between Hα luminosity and M_st for the models DDC0, DDC15, and DDC25 at 100, 150, 200, 250, and 300 d.

Model	Age [d]	a₀	a₁	a₂
DDC0	100	39.15	−0.01	−0.10
DDC0	150	39.34	−0.05	−0.17
DDC0	200	39.35	0.04	−0.21
DDC0	250	39.25	0.19	−0.21
DDC0	300	39.04	0.29	−0.21
DDC15	100	39.11	−0.02	−0.10
DDC15	150	39.31	−0.02	−0.16
DDC15	200	39.30	0.07	−0.20
DDC15	250	39.16	0.15	−0.24
DDC15	300	38.97	0.30	−0.22
DDC25	100	39.01	−0.01	−0.09
DDC25	150	39.22	0.06	−0.14
DDC25	200	39.19	0.17	−0.17
DDC25	250	39.01	0.22	−0.21
DDC25	300	38.79	0.37	−0.18

Notes. The polynomial has the formY = a₀ + a₁X + a₂X², where Y = log₁₀(L(Hα)_diff/erg s⁻¹) and X = log₁₀(M_st∕M_⊙).

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.