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A Spectroscopic Study of the Rich Supernova Remnant Population in M83

  • Authors: P. Frank Winkler, William P. Blair, and Knox S. Long

2017 The Astrophysical Journal 839 83.

  • Provider: AAS Journals

Caption: Figure 10.

Plots showing the flux ratio [O III] λ 5007/Hβ, as a function of the following other line ratios for M83 SNRs, and also for ones in M31 (Galarza et al. 1999) and M81 (Lee et al. 2015): (left) [N II] λ 6583/Hα ratio; (center) [O I] λ 6300/Hα ratio; (right) [S II] λλ 6716, 6731/Hα ratio. These plots can be compared with corresponding figures in the shock modeling paper of Allen et al. (2008).

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