Can A Kinematically Hot and Thick Disk Form A Bar? : Role of Highly Spinning Dark Matter Halos

This article explores the relationship between the formation of galactic bars and the properties of dark matter halos, specifically focusing on the role of highly spinning halos. The research likely investigates how the dynamics of these halos influence the stability and evolution of galactic disks, and whether the presence of such halos can facilitate or hinder the formation of bar structures. The use of 'kinematically hot and thick disk' suggests the study considers disks with significant internal motion and vertical extent, which are common in galaxies.