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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 l...

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Main Authors: Korth J., Mustill A. J., Parviainen H., Villaver E., Kuehne J. W., Béjar V. J. S., Hayashi Y., Abreu García N., Kagetani T., Kawauchi K., Livingston L., Mori M., Morello G., Watanabe N., Fukuda I., Ikuta K., Bonilla-Mariana I., Esparza-Borges E., Fernández-Rodríguez G., Fukui A., Geraldía-González S., González-Rodríguez J., Isogai K., Narita N., Palle E., Peláez-Torres A., Sánchez-Benavente M.
Format: Artigo
Language:Inglês
Published: EDP Sciences 2026-05-01
Series:Astronomy & Astrophysics
Subjects:
techniques: photometric
stars: individual: wd 1054-226
white dwarfs
Online Access:https://www.aanda.org/articles/aa/full_html/2026/05/aa58102-25/aa58102-25.html
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