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• W3100877462 endingPage "127" @default.
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• W3100877462 abstract "Core-collapse supernova (SN) explosions expose the structure and environment of massive stars at the moment of their death. We use the global fitting technique of Pejcha & Prieto to estimate a set of physical parameters of 19 normal SNe II, such as their distance moduli, reddenings, 56Ni masses , and explosion energies from multicolor light curves and photospheric velocity curves. We confirm and characterize known correlations between and bolometric luminosity at 50 days after the explosion, and between and . We pay special attention to the observed distribution of coming from a joint sample of 38 SNe II, which can be described as a skewed-Gaussian-like distribution between and , with a median of , mean of , standard deviation of , and skewness of 3.050. We use a two-sample Kolmogorov–Smirnov test and two-sample Anderson–Darling test to compare the observed distribution of to results from theoretical hydrodynamical codes of core-collapse explosions with the neutrino mechanism presented in the literature. Our results show that the theoretical distributions obtained from the codes tested in this work, KEPLER and Prometheus Hot Bubble, are compatible with the observations irrespective of different pre-SN calibrations and different maximum mass of the progenitors." @default.
• W3100877462 created "2020-11-23" @default.
• W3100877462 creator A5045282670 @default.
• W3100877462 creator A5048301562 @default.
• W3100877462 creator A5067881179 @default.
• W3100877462 creator A5077644188 @default.
• W3100877462 date "2017-06-05" @default.
• W3100877462 modified "2023-09-23" @default.
• W3100877462 title "The Nickel Mass Distribution of Normal Type II Supernovae" @default.
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• W3100877462 doi "https://doi.org/10.3847/1538-4357/aa72f1" @default.
• W3100877462 hasPublicationYear "2017" @default.
• W3100877462 type Work @default.

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