Constraints on environs around SN 2011fe and SN 2014J from radio modeling and observations
Abstract
The radio non-detection of two Type Ia supernovae (SNe) SN 2011fe and SN 2014J has been modeled considering synchrotron radiation from shock accelerated electrons in the SN shock fronts. With 10% each of the bulk kinetic energy in electric and magnetic fields, a very low density of the medium around both the SNe has been estimated from the null detection of radio emission, around 1 and 4 years after the explosion of SNe 2014J and 2011fe, respectively. Keeping the fraction of energy in electrons fixed at 10%, a medium with particle density ~ 1cm-3 is found when 1% of the post shock energy is in magnetic fields. In case of a wind medium, the former predicts the mass loss rate Ṁ to be <10-9 M ⊙ yr-1, and the latter gives an upper limit ~10-9 M ⊙ yr-1, for wind velocity of 100 kms-1, for both the SNe. The tenuous media obtained from this study favor the double degenerate as well as a spin up/down model for both SNe 2011fe and 2014J.
- Publication:
-
Supernova 1987A:30 years later - Cosmic Rays and Nuclei from Supernovae and their Aftermaths
- Pub Date:
- February 2017
- DOI:
- 10.1017/S1743921317005300
- Bibcode:
- 2017IAUS..331...69K
- Keywords:
-
- stars: circumstellar matter;
- supernovae: general;
- supernovae: individual (SN 2011fe;
- SN 2014J)