well known that as they evolve, large voids tend to be rounder, a behaviour which is opposite to that shown by bound structure. Negative density perturbations in the initial fluctuation field that will later become voids, are characterised by a decreasing asphericity as the expansion of the Universe proceeds, as is shown by @Sheth1 (and references therein). Taking advantage of this particular characteristic of voids, it is possible to study the whether galaxy or halo angular momenta are aligned with the void shells just by considering the angle with respect to the direction to the void centre. This is the approach used by @Trujillo1 applied to the SDSS and 2dFGRS galaxy redshift surveys, and by @Brunino1, @Cuesta1 and @Patiri1 to numerical simulations. @Trujillo1 find with a high level of confidence that spiral galaxies located on the shells of the largest cosmic voids have rotation axes that lie preferentially on the void surface, in agreement with the simulation results of @Brunino1 [@Cuesta1; @Patiri1]. Other more general methods that also take into account alignments with large scale filaments in numerical simulations show similar results [@Aragon1; @Hahn1; @Hahn2].

In this paper we present results from a study of alignments between individual objects and 