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Thermal and Nonthermal Emission at Large Radii in the ... - HEASARC

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Tighter
Limit
from
XIS
(Cont.)<br />

• Assume
same
spectral
<strong>in</strong>dex
<strong>at</strong>
lower
energies<br />

• Assume
XIS
=
<strong>the</strong>rmal
+
IC<br />

• Assume
IC
follows
radio
image<br />

• Apply
results
to
all
of
relic<br />

F X 


2.2

µG,
very
strong
magnetic
field
<strong>at</strong>
<br />

projected
radius
of
~2
Mpc
!!<br />

Some
previous
evidence
for
a
strong
B
<strong>in</strong>
relic
from<br />

Faraday
rot<strong>at</strong>ion
(Johnston-Hollitt
2004).

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