  We apply the Keski-Vakkuri, Kraus and Wilczek (KKW) generalized analysis to a
magnetic stringy black hole solution to compute its temperature and entropy.
The solution that we choose in the Einstein-dilaton-Maxwell theory is the dual
solution known as the magnetic black hole solution. Our results show that the
expressions of the temperature and entropy of this non-Schwarzschild-type black
hole are not the Hawking temperature and the Bekenstein-Hawking entropy,
respectively. In addition, the extremal magnetic stringy black hole is not
frozen because it has a constant non-zero temperature.
