LISA sources in globular clusters

Globular clusters house a population of compact binaries that will be inter esting gravitational wave sources for LISA.. We provide estimates for the n umbers of sources of several categories and discuss the sensitivity of LISA to detecting these sources. The estimated total number of detectable sourc es ranges from similar to 10 to similar to 10(3) with gravitational wave fr equencies above 1 mHz. These sources are typically undetectable by any othe r means and thus offer an opportunity for doing true gravitational-wave ast ronomy. The detection of these sources would provide information about both binary star evolution and the dynamics of globular clusters.