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A magnetic white dwarf formed through a binary merger within 35 million years
ref [9] · 2509.01069 · notice #8534 · dispute
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each with different initial periods, resulting in WD masses that vary accordingly (thus the color represents only the outcome for one of the periods). Bergeron, P., Leggett, S. K., & Ruiz, M. T. 2001, The Astrophysical Journal Supplement Series, 133, 413, doi: 10.1086/320356 Bouma, L. G., Kerr, R., Curtis, J. L., et al. 2022, The Astronomical Journal, 164, 215, doi: 10.3847/1538-3881/ac93ff Briggs, G. P., Ferrario, L., Tout, C. A., Wickramasinghe, D. T., & Hurley, J. R. 2015, MNRAS, 447, 1713, doi: 10.1093/mnras/stu2539 Bruzual A., G. 2010, Philosophical Transactions of the Royal Society of London Series A, 368, 783, doi: 10.1098/rsta.2009.0258 Caiazzo, I., Burdge, K. B., Fuller, J., et al. 2021, Natur, 595, 39, doi: 10.1038/s41586-021-03615-y