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We study a six-dimensional vector-tensor gravitation theory compactified toM_4 x S^2. Here, static spherically-symmetric solutions to the field equationsof the theory are investigated. We examine the case that the magnetic charge ofthe "black hole" is small compared with that located in the "center" of theextra sphere. The Hawking temperature of the black hole is calculated in asimple case.

Charged black holes in a six-dimensional vector-tensor theory