WD 1054-226 revisited: A stable transiting debris system
Context. A growing number of white dwarfs (WDs) exhibit one or more signs of remnant planetary systems, including transits, infrared excesses, and atmospheric metal pollution. WD 1054-226 stands out for its unique, highly structured, and persistent photometric variability.Aims. We investigate the long-term stability and nature of the periodic signals observed in WD 1054-226 to better understand th
