Fig. 2 from Generalizations of the Tully‐Fisher Relation for Early‐ and Late‐Type Galaxies

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Generalizations of the Tully‐Fisher Relation for Early‐ and Late‐Type Galaxies

Authors: Sven De Rijcke, Werner W. Zeilinger, George K. T. Hau, P. Prugniel, and Herwig Dejonghe

De Rijcke et al. 2007 The Astrophysical Journal 659 1172.

Provider: AAS Journals

Caption: Fig. 2.

Left: Stellar mass Tully‐Fisher relation. Symbols same as in Fig. 1 (with spiral = TP00+M05+G06). Right: H I gas+stellar mass Tully‐Fisher relation. For the late types, only M05 and G06 give all the necessary ingredients to derive ﹩M_{g+s}﹩, so spiral = M05+G06 here.

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