Fig. 3 from Late‐Time Observations of SN 2006gy: Still Going Strong

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Late‐Time Observations of SN 2006gy: Still Going Strong

Authors: Nathan Smith, Ryan J. Foley, Joshua S. Bloom, Weidong Li, Alexei V. Filippenko, Raphaël Gavazzi, Andrea Ghez, Quinn Konopacky, Matthew A. Malkan, Philip J. Marshall, David Pooley, Tommaso Treu, and Jong-Hak Woo

Smith et al. 2008 The Astrophysical Journal 686 485.

Provider: AAS Journals

Caption: Fig. 3.

Observed spectrum at the position of SN 2006gy on day 364 after explosion. The SN position is halfway between the two dashed lines. Continuum from the nucleus of NGC 1260 is seen clearly, as is the narrow Hα and [N II] emission from H II regions that follow the galaxy’s rotation curve. We detect no broad or intermediate‐width Hα emission from SN 2006gy.

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