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The structure of the Taurid meteor complex based on photographic orbitsavailable in the IAU Meteor database is studied. We have searched for potentialsub-streams or filaments to be associated with the complex utilizing theSouthworth-Hawkins D-criterion. Applying a strict limiting value for D=0.10,fifteen sub-streams or filaments, consisting of more than three members, couldbe separated out from the general complex. To confirm their mutual consistenceas filaments, rather than fortuitous clumping at the present time, the orbitalevolution over 5000 years of each member is studied. Utilizing the D-criterionwe also searched for NEOs that might be associated with the streams andfilaments of the complex and investigated the orbital evolution of potentialmembers. Possible associations between 7 Taurid filaments and 9 NEOs werefound. The most probable are for S Psc(b) -- 2003QC10, N Tau(a) -- 2004TG10, oOri -- 2003UL3 and N Tau(b) -- 2002XM35. Some of the potential parent objectscould be either dormant comets or larger boulders moving within the complex.Three of the most populated filaments of the complex may have originated from2P/Encke.

The Taurid complex meteor showers and asteroids