So Great Is Their Love

A soundscape composition intended for installation in a sound art exhibition. This short project is a contribution to practice-led research that questions that nature of authorial identity, and the composer's responsibility for the sounds produced. First made public in The Braid, Ballymena, 25 September 2013

The not-so-extreme white dwarf of the CV GD 552

GD 552 is a cataclysmic binary which was previously believed to be composed of an M-star and a white dwarf, the latter having an extreme mass of 1.4 solar masses. In a recent paper we showed that this is not compatible with new observational evidence and presented an alternative model in which the white dwarf has a typical mass and the companion is a brown dwarf, making the system a likely member of the elusive group of CVs which have already evolved through minimum orbital period. Here we present additional spectroscopical evidence supporting this conclusion by means of skew mapping.