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We review the properties of Galactic binaries containing two compact objects,as derived by means of population synthesis. Using this information wecalculate the gravitational wave signal of these binaries. At frequencies belowf ~< 2 mHz the double white dwarf population forms an unresolved background forthe low-frequency gravitational wave detector LISA. Above this limit some fewthousand double white dwarfs and few tens of binaries containing neutron starswill be resolved. Of the resolved double white dwarfs ~500 have a total massabove the Chandrasekhar limit. About ~95 of these have a measurable frequencychange allowing a determination of their chirp mass. We discuss the propertiesof the resolved systems.

The gravitational wave signal from the Galactic disk population of binaries containing two compact objects