Born-Again Protoplanetary Disk around Mira B

@article{Ireland2007BornAgainPD,
  title={Born-Again Protoplanetary Disk around Mira B},
  author={Michael J. Ireland and John D. Monnier and Peter G. Tuthill and Richard W. Cohen and James M. De Buizer and Christopher Packham and David R. Ciardi and Thomas L. Hayward and James P. Lloyd},
  journal={The Astrophysical Journal},
  year={2007},
  volume={662},
  pages={651-657}
}
The Mira AB system is a nearby (~107 pc) example of a wind accreting binary star system. In this class of system, the wind from a mass-losing red giant star (Mira A) is accreted onto a companion (Mira B), as indicated by an accretion shock signature in spectra at ultraviolet and X-ray wavelengths. Using novel imaging techniques, we report the detection of emission at mid-infrared wavelengths between 9.7 and 18.3 µm from the vicinity of Mira B but with a peak at a radial position about 10 AU… 

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