2016ApJ...833..147L

Due to its proximity, SN 1987A offers a unique opportunity to directly observe the geometry of a stellar explosion as it unfolds. Here we present spectral and imaging observations of SN 1987A obtained ∼10,000 days after the explosion with HST/STIS and VLT/SINFONI at optical and near-infrared wavelengths. These observations allow us to produce the most detailed 3D map of Hα to date, the first 3D maps for [Ca ii]
lambdaλ7292,7324, [O i]
lambdaλ6300,6364, and Mg ii
lambdaλ9218,9244, as well as new maps for [Si i]+[Fe ii]\1.644
mum and He i 2.058 µm. A comparison with previous observations shows that the [Si i]+[Fe ii] flux and morphology have not changed significantly during the past ten years, providing evidence that this line is powered by ⁴⁴Ti. The time evolution of Hα shows that it is predominantly powered by X-rays from the ring, in agreement with previous findings. All lines that have sufficient signal show a similar large-scale 3D structure, with a north-south asymmetry that resembles a broken dipole. This structure correlates with early observations of asymmetries, showing that there is a global asymmetry that extends from the inner core to the outer envelope. On smaller scales, the two brightest lines, Hα and [Si i]+[Fe ii] 1.644 µm, show substructures at the level of ∼200-1000 km s^–1and clear differences in their 3D geometries. We discuss these results in the context of explosion models and the properties of dust in the ejecta.