Fig. 6 from The Observability of Abundance Ratio Effects in Dynamically Hot Stellar Systems

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The Observability of Abundance Ratio Effects in Dynamically Hot Stellar Systems

Authors: Jedidiah Serven, Guy Worthey, and Michael M. Briley

Serven, Worthey, & Briley 2005 The Astrophysical Journal 627 754.

Provider: AAS Journals

Caption: Fig. 6.

Cr3594 index (horizontal lines). The Cr‐enhanced (dotted curve) and normal (solid curve) spectra are overplotted near the bottom with scale to the right. The ratio of the two spectra are shown (dashed curve) at the top, with scale to the left.

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