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Conclusions<br />
1. The Milky Way has larger amplitude<br />
m=0,1,2 modes in the HI mean plane<br />
at R > R 0. Higher order modes are<br />
much weaker.<br />
2. The m=0 mode implies that the Galaxy<br />
is moving through a hot IGM.<br />
3. Many galaxies may have these modes.<br />
4. Looking for DM halos by this method<br />
probably won’t work.
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