paper

A New Evolutionary Phase of Supernova Remnant 1987A

arXiv:1104.4825 · doi:10.1088/2041-8205/733/2/L35

Abstract

We have been monitoring the supernova remnant (SNR) 1987A with {\it Chandra} observations since 1999. Here we report on the latest change in the soft X-ray light curve of SNR 1987A. For the last 1.5 yr (since day 8000), the soft X-ray flux has significantly flattened, staying (within uncertainties) at 5.7 10 erg cm s (corresponding to 3.6 10 erg s) in the 0.5--2 keV band. This remarkable change in the recent soft X-ray light curve suggests that the forward shock is now interacting with a decreasing density structure, after interacting with an increasing density gradient over 10 yr prior to day 8000. Possibilities may include the case that the shock is now propagating beyond a density peak of the inner ring. We briefly discuss some possible implications on the nature of the progenitor and the future prospects of our {\it Chandra} monitoring observations.

11 pages, 2 tables, 1 color figure, Accepted by ApJ Letters

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