For more than a century, the binary star system ε Aurigae has been a riddle, wrapped in a mystery, inside an enigma. But no more — the system's previously inferred but unseen disk of dust has been detected.
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References
Kloppenborg, B. et al. Nature 464, 870–872 (2010).
Goodricke, J. Phil. Trans. R. Soc. 73, 474–482 (1783).
Guinan, E. F. & DeWarf, L. Astron. Soc. Pacif. Conf. Ser. 279, 121–142 (2002).
Lissauer, J. J., Wolk, S. J., Griffith, C. A. & Backman, D. E. Astrophys. J. 465, 371–384 (1996).
Huang, S.-S. Astrophys. J. 141, 976–984 (1965).
Hoard, D. W., Howell, S. B. & Stencel, R. E. Preprint at http://arxiv.org/abs/1003:3694 (2010).
Carroll, S. M., Guinan, E., McCook, G. & Donahue, R. Astrophys. J. 367, 278–287 (1991).
Webbink, R. F. NASA Conf. Publ. 2384, 49–59 (1985).
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Guinan, E. Shrouded in a dusty disk. Nature 464, 842–843 (2010). https://doi.org/10.1038/464842a
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DOI: https://doi.org/10.1038/464842a