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[O I] λλ6300, 6364 in the Nebular Spectrum of a Subluminous Type Ia Supernova

  • Authors: S. Taubenberger, M. Kromer, R. Pakmor, G. Pignata, K. Maeda, S. Hachinger, B. Leibundgut, and W. Hillebrandt

Taubenberger et al. 2013 The Astrophysical Journal Letters 775 L43.

  • Provider: AAS Journals

Caption: Figure 2.

Profile of the [O i] λλ6300, 6364 line in SN 2010lp, and its reproduction—within the Gauss-fitting approach of Taubenberger et al. (2009)—as a double-peaked structure atop a broad base. The narrow components have velocity offsets of ~ ± 1900 km s −1 from the rest position, and FWHM velocities of ~1700 km s −1.

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