Late-time photometry of type Ia supernova SN 2012cg reveals the radioactive decay of ⁵⁷Co
Seitenzahl et al. have predicted that roughly three years after its explosion, the light we receive from a Type Ia supernova (SN Ia) will come mostly from reprocessing of electrons and X-rays emitted by the radioactive decay chain ⁵⁷Co → ⁵⁷Fe, instead of positrons from the decay chain ⁵⁶Co → ⁵⁶Fe that dominates the SN light at earlier times. Using the Hubble Space Telescope, we followed the light curve of the SN Ia SN 2012cg out to 1055 days after maximum light. Our measurements are consistent...[Show more]
|Collections||ANU Research Publications|
|Source:||The Astrophysical Journal|
|01_Graur_Late-Time_Photometry_2016.pdf||1.24 MB||Adobe PDF|
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