Abstract
We present an analysis of Murchison Widefield Array radio telescope data from
$ømega$ Cen, possibly a stripped dwarf spheroidal galaxy core captured by our
Galaxy. Recent interpretations of Fermi-LAT $\gamma$-ray data by Brown et
al. (2019) and Reynoso-Cordova et al. (2019) suggest that $ømega$ Cen
may contain significant Dark Matter. We utilise their best-fit Dark Matter
annihilation models, and an estimate of the magnetic field strength in $ømega$
Cen, to calculate the expected radio synchrotron signal from annihilation, and
show that one can usefully rule out significant parts of the magnetic field -
diffusion coefficient plane using the current observational limits. Improvement
by a factor of 10-100 on these limits could constrain the models even more
tightly.
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