Bibcode
                                    
                            Kilic, Mukremin; Brown, W. R.; Kenyon, S. J.; Allende Prieto, C.
    Bibliographical reference
                                    American Astronomical Society, AAS Meeting #217, #423.02; Bulletin of the American Astronomical Society, Vol. 43, 2011
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                        2011
            
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                            Description
                                    Short period binary white dwarfs may merge within a Hubble time due to
gravitational wave radiation. We have begun a targeted survey to find
merging white dwarfs systems, and our first results have tripled the
number of known merging white dwarf systems. Our sample includes systems
with orbital periods as short as 1 hr and with merger times less than
100 Myr. We will discuss the characteristics of
this merger sample and potential links to Type Ia and underluminous
supernovae.