क्यूआर कोड

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...

पूर्ण विवरण

में बचाया:
मुख्य लेखकों: 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.
स्वरूप: Artigo
भाषा:Inglês
प्रकाशित: EDP Sciences 2026-05-01
श्रृंखला:Astronomy & Astrophysics
विषय:
techniques: photometric
stars: individual: wd 1054-226
white dwarfs
ऑनलाइन पहुंच:https://www.aanda.org/articles/aa/full_html/2026/05/aa58102-25/aa58102-25.html
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