A Mid-life crisis? Sudden Changes in Radio and X-Ray Emission from Supernova 1970G

Jason A Dittmann, Alicia M. Soderberg, Laura Chomiuk, Raffaella Margutti, W. M. Goss, Dan Milisavljevic, Roger A. Chevalier

Published 2014-03-26, updated 2014-03-29Version 2

Supernovae provide a backdrop from which we can probe the end state of stellar evolution in the final years before the progenitor star explodes. As the shock from the supernova expands, the timespan of mass loss history we are able to probe also extends, providing insight to rapid time-scale processes that govern the end state of massive stars. While supernovae transition into remnants on timescales of decades to centuries, observations of this phase are currently limited. Here we present observations of SN 1970G, serendipitously observed during the monitoring campaign of SN 2011fe that shares the same host galaxy. Utilizing the new Jansky Very Large Array upgrade and a deep X-ray exposure taken by the Chandra Space Telescope, we are able to recover this middle-aged supernova and distinctly resolve it from the HII cloud with which it is associated. We find that the flux density of SN 1970G has changed significantly since it was last observed - the X-ray luminosity has increased by a factor of ~3, while we observe a significantly lower radio flux of only 27.5 micro-Jy at 6.75 GHz, a level only detectable through the upgrades now in operation at the Jansky Very Large Array. These changes suggest that SN 1970G has entered a new stage of evolution towards a supernova remnant, and we may be detecting the turn-on of the pulsar wind nebula. Deep radio observations of additional middle-aged supernovae with the improved radio facilities will provide a statistical census of the delicate transition period between supernova and remnant.