Figure 5 from Thermonuclear .Ia Supernovae from Helium Shell Detonations: Explosion Models and Observables

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Thermonuclear .Ia Supernovae from Helium Shell Detonations: Explosion Models and Observables

Authors: Ken J. Shen, Dan Kasen, Nevin N. Weinberg, Lars Bildsten, and Evan Scannapieco

SHEN et al. 2010 The Astrophysical Journal 715 767.

Provider: AAS Journals

Caption: Figure 5.

Multiband light curves for the 0.6 + 0.2 M _☉ model in Vega magnitudes. The dashed line shows the bolometric light curve, and the solid lines show magnitudes for various filters as labeled. The secondary peak in redder wavebands is apparent beginning sime 15 days after explosion, which is sime 7 days after the time of B-band maximum.

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