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We obtain the general solution for non-extremal 3-charge dilatonic rotatingblack holes in the U(1)^3 gauged five-dimensional N=2 supergravity coupled totwo vector multiplets, in the case where the two rotation parameters are setequal. These solutions encompass all the previously-known extremal solutions,and, by setting the three charges equal, the recently-obtained non-extremalsolutions of N=2 gauged five-dimensional pure supergravity.Comment: 8 pages, Latex. Statements about extra parameter \gamma corrected to  reflect the fact that it is trivia

physical review. d. particles, fields, gravitation, and cosmology/physical review. d, particles, fields, gravitation, and cosmology

Charged rotating black holes in five dimensional<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="normal">U</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mn>1</mml:mn><mml:msup><mml:mo stretchy="false">)</mml:mo><mml:mn>3</mml:mn></mml:msup></mml:math>gauged<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="script">N</mml:mi><mml:mo>=</mml:mo><mml:mn>2</mml:mn></mml:math>supergravity

Charged rotating black holes in five dimensionalU(1)3gaugedN=2supergravity