All three 2003fg-like supernovae show correlated asymmetries in their 1.257 and 1.644 micron [Fe II] profiles, implying aspherical chemical distributions in their cores.
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Using nebular near-IR spectroscopy to measure asymmetric chemical distributions in 2003fg-like thermonuclear supernovae
All three 2003fg-like supernovae show correlated asymmetries in their 1.257 and 1.644 micron [Fe II] profiles, implying aspherical chemical distributions in their cores.