  The three young clusters in the Galactic Center represent the closest
examples of massive starbursts and they define the upper mass limit of the
Galactic cluster mass functions. In this review, I describe the characteristics
and content of the Arches, Quintuplet, and Central clusters. They each are more
massive than any other cluster in the Galaxy, and the Arches cluster, in
particular, has a mass and age that make it ideal for studies of massive
stellar evolution and dense stellar systems. A preliminary measurement
indicates that the initial mass function in the Galactic center is top-heavy,
suggesting an environmental effect that has otherwise been absent in similar
observations for Galactic clusters. Given the relatively more evolved nature of
the Quintuplet and Central clusters, these clusters contain stars in a wide
range of evolutionary states, including Luminous Blue Variables and Wolf-Rayet
stars. The Quintuplet cluster provides a particularly interesting view of the
most massive stars that are known, the Pistol Star and FMM362. An analysis of
the mass spectrum in the Arches cluster suggests an upper mass cutoff of
\~150-200 Msun.
