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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. 9.

Ti5000 index (horizontal lines). The Ti‐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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