Radio view of a broad-line Type Ic supernova ASASSN-16fp
arXiv:2003.02709 · doi:10.1093/mnras/staa700
Abstract
We present extensive radio observations of a Type Ic supernova, ASASSN-16fp. Our data represents the lowest frequency observations of the SN beyond 1000 days with a frequency range of GHz and a temporal range of 8 to 1136 days post-explosion. The observations are best represented by a model of synchrotron emission from a shocked circumstellar shell initially suppressed by synchrotron self-absorption. Assuming equipartition of energy between relativistic particles and magnetic fields, we estimate the velocity and radius of the blast wave to be and cm respectively at 8 days post-explosion. We infer the total internal energy of the radio-emitting material evolves as 0.37 (t/t) erg. We determine the mass-loss rate of the progenitor star to be at various epochs post-explosion, consistent with the mass-loss rate of Galactic Wolf-Rayet stars. The radio light curves and spectra show a signature of density enhancement in the CSM at a radius of cm from the explosion center.
arXiv comment14 pages, 7 figures, Accepted for publication in MNRAS
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