Fig. 2 from Dynamically Close Galaxy Pairs and Merger Rate Evolution in the CNOC2 Redshift Survey

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Dynamically Close Galaxy Pairs and Merger Rate Evolution in the CNOC2 Redshift Survey

Authors: D. R. Patton, C. J. Pritchet, R. G. Carlberg, R. O. Marzke, H. K. C. Yee, P. B. Hall, H. Lin, S. L. Morris, M. Sawicki, C. W. Shepherd, and G. D. Wirth

Patton et al. 2002 The Astrophysical Journal 565 208.

Provider: AAS Journals

Caption: Fig. 2.

Model k‐corrections from Coleman et al. (1980) are given for four galaxy types. Lines are as follows: E/S0 (long‐dashed line), Sbc (dashed line), Scd (dotted line), and Im (solid line). The maximal k‐correction ﹩k^{\mathrm{max}\,}_{R_{\mathrm{C}\,}\rightarrow B}( z) ﹩ is marked with a thick dashed line.

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