New Techniques For Relating Dynamically Close Galaxy Pairs to Merger and Accretion Rates: Application To The SSRS2 Redshift Survey

Accepted For Publication In The Astrophysical Journal

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Abstract

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SSRS2 Pair Classification Experiment

This link provides access to a clickable version of Figure 5. This allows the user to bring up the image for any of the 255 SSRS2 pairs with projected separation rp < 100/h kpc, providing an intuitive feel for the strength and prevalence of signs of interaction, as a function of rp and line-of-sight separation (). For best results, make your browser fill as much of your screen as possible.

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Last modified: Thursday Jan. 20 11:37, 2000