File:SNIacurva.png

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Summary

DescriptionSNIacurva.png	English: The radioactive decays of nickel-56 and cobalt-56 that produce a supernova visible light curve.
Date	4 September 2005 (original upload date)
Source	No machine-readable source provided. Own work assumed (based on copyright claims). References: Hillebrandt, W. (2000). "Type IA Supernova Explosion Models". Annual Review of Astronomy and Astrophysics 38 (1): 191–230. DOI:10.1146/annurev.astro.38.1.191. Mazzali, P. A. (2001). "Can Differences in the Nickel Abundance in Chandrasekhar‐Mass Models Explain the Relation between the Brightness and Decline Rate of Normal Type Ia Supernovae?". The Astrophysical Journal 547 (2): 988. DOI:10.1086/318428.
Author	No machine-readable author provided. Xenoforme~commonswiki assumed (based on copyright claims).

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