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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Hlavní autoři:	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.
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	EDP Sciences 2026-05-01
Edice:	Astronomy & Astrophysics
Témata:	techniques: photometric stars: individual: wd 1054-226 white dwarfs
On-line přístup:	https://www.aanda.org/articles/aa/full_html/2026/05/aa58102-25/aa58102-25.html
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