imageAmendment 1 published on 5 December 2003
Description:

The definitions of the high mass and low mass white dwarf binaries from [31] were switched. This has been corrected.


Old version:

There are four classes of relativistic binaries that are brought into contact by gravitational radiation: low mass white dwarf-white dwarf binaries (2 WD a) with total mass below the Chandrasekhar mass; high mass white dwarf-white dwarf binaries (WD2b) with total mass above the Chandrasekhar mass; neutron star-white dwarf binaries (NW); and neutron star-neutron star binaries NS2


Author's comment: Typographical error


Editorial comment: Amendment requested by author on 19 Nov 2003