AAS 207th Meeting, 8-12 January 2006
Session 126 Dark Matter, Dark Energy and Neutrinos
Poster, Wednesday, 9:20am-6:30pm, January 11, 2006, Exhibit Hall

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[126.04] Galactic Interactions and Dark Matter

T. Willig, A. Storrs (Towson Univ.)

In studying galactic interactions is it possible with present instrumentation to find evidence of dark matter within these interactions? The present theory is that dark matter and its gravitational force is what accounts for much of spiral galaxy rotation curves. If this is true, we should be able to find evidence of dark matter when two galaxies (one being a spiral galaxy) interact. Several pairs of interacting galaxies in various stages of interaction will be studied. In addition, several non interacting spiral galaxies will be studied for comparisons.

We present analysis of a variety of archival imaging data from radio maps through x-ray images in an attempt to observe the effects of dark matter in galaxy interactions.

The author(s) of this abstract have provided an email address for comments about the abstract: timwillig@yahoo.com

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