We report on the present stage of SN 1987A as observed by the Chandra X-Ray Observatory. We reanalyze published Chandra observations and add three more epochs of Chandra data to get a consistent picture of the evolution of the X-ray fluxes in several energy bands. We discuss the implications of several calibration issues for Chandra data. Using the most recent Chandra calibration files, we find that the 0.5-2.0 keV band fluxes of SN 1987A have increased by ∼6 × 10-13 erg s-1 cm-2 per year since 2009. This is in contrast with our previous result that the 0.5-2.0 keV light curve showed a sudden flattening in 2009. Based on our new analysis, we conclude that the forward shock is still in full interaction with the equatorial ring. © 2013. The American Astronomical Society. All rights reserved..
CITATION STYLE
Helder, E. A., Broos, P. S., Dewey, D., Dwek, E., McCray, R., Park, S., … Burrows, D. N. (2013). Chandra observations of SN 1987A: The soft X-ray light curve revisited. Astrophysical Journal, 764(1). https://doi.org/10.1088/0004-637X/764/1/11
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