A Three-dimensional Map Of Interstellar Dust In Front Of SN 1987A

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

Light echoes from supernovae can illuminate interstellar dust and provide information on its structure, composition, and density. We have developed a new difference imaging technique (Newman & Rest 2006) for extracting light echo fluxes from a series of observations, without the need for an echo-free template. Using this method, along with 5 years of SuperMACHO imaging, we have obtained deep and detailed images of the light echoes around SN 1987A. Light echo positions are identified in these images using an automated flux-peak detection algorithm. Knowing the position on the sky and the epoch of observation, we obtain the three-dimensional position of the reflecting dust. Our dust maps show three extended structures with varying inclinations, along with a variety of filamentary strands extending 1.2 kpc in the supernova foreground. These maps will be valuable for studying the geometry and evolution of superbubbles in the Large Magellanic Cloud.

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