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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Cited by in corpus (14)
- Chandra Observes the End of an Era SN 1987A
- The morphology of the ejecta in Supernova 1987A: a study over time and wavelength
- Chandra observations of SN 1987A: the soft X-ray light curve revisited
- High-resolution radio observations of SNR 1987A at high frequencies
- Late Spectral Evolution of the Ejecta and Reverse Shock in SN1987A
- HST-COS Observations of Hydrogen, Helium, Carbon and Nitrogen Emission from the SN 1987A Reverse Shock
- The 30-Year Search for the Compact Object in SN 1987A
- Recovery of the Historical SN1957D in X-rays with Chandra
- XMM-Newton observations of SNR 1987A. II. The still increasing X-ray light curve and the properties of Fe K lines
- Thermal Emission and Radioactive Lines, but No Pulsar, in the Broadband X-Ray Spectrum of Supernova 1987A
- Spectral Evolution of the X-Ray Remnant of SN 1987A: A High-Resolution HETG Study
- High-cadence Dispersed Spectral Analysis of Supernova Remnant 1987A
- Latest Evolution of the X-Ray Remnant of SN 1987A: Beyond the Inner Ring
- Polarized radio emission unveils the structure of the pre-supernova circumstellar magnetic field and the radio emission in SN1987A