Double-detonation sub-Chandrasekhar supernovae: can minimum helium shell masses detonate the core?

M. Fink; F. K. Röpke; W. Hillebrandt; I. R. Seitenzahl; S. A. Sim; M. Kromer

doi:10.1051/0004-6361/200913892

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Volume 514 (May 2010)

A&A, 514 (2010) A53

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Table 4:

Rise times $t_{\rm peak}$ and peak absolute magnitudes $M_{\rm peak}^{\rm bol}$ for the UVOIR bolometric light curves of the models.
Model	1	2	3	4	5	6
$t_{\rm peak}$ [days]	18.6	18.6	18.0	15.5	14.4	13.9
$M_{\rm peak}^{\rm bol}$	-17.6	-18.2	-18.7	-19.1	-19.4	-19.5
$\Delta m_{15}^{\rm bol}$	0.64	0.40	0.50	0.55	0.55	0.66

Notes. $\Delta m_{15}^{\rm bol}$ is the change in bolometric magnitude between maximum light and 15 days thereafter. Due to Monte Carlo noise magnitudes are uncertain by $\sim$ 0.1 mag.

Source LaTeX | All tables | In the text

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