Why a ring of stars at r = 20 kpc?
Abstract
Description
The recently discovered ring of stars near Galactocentric distance $r = 20$ kpc is interpreted as baryonic matter accreted onto the second caustic ring of dark matter in our galaxy. Caustic rings of dark matter were predicted in the Galactic plane at radii $a_n \simeq 40 kpc/n$ where $n=1,2,3 ..$. They can reveal themselves by their gravitational influence on the distribution of baryonic matter. There is additional evidence for caustic rings of dark matter in the Milky Way from a series of sharp rises in the Galactic rotation curve. The positions of the rises are consistent at the 3% level with the above law for the caustic ring radii. Also, a triangular feature in the IRAS map of the galactic plane is consistent with the imprint of the caustic ring of dark matter nearest to us ($n=5$) upon dust and gas in the Galactic plane. These observations imply that the dark matter in our neighborhood is dominated by a single flow whose density and velocity vector are estimated.
12 pages, 3 figures, invited talk at the Beyond '03 Conference on Physics beyond the Standard Model, Castle Ringberg, Tegernsee, Germany, June 9 - 14, 2003
12 pages, 3 figures, invited talk at the Beyond '03 Conference on Physics beyond the Standard Model, Castle Ringberg, Tegernsee, Germany, June 9 - 14, 2003