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Cited article:

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THE STRUCTURE AND KINEMATICS OF THE ENVELOPE AROUND U ORI FROM IOTA OBSERVATIONS

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Characterization of Dust Shell Dynamics and Asymmetry for Six Mira‐Type Stars

K. Tatebe, A. A. Chandler, D. D. S. Hale and C. H. Townes
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First Surface‐resolved Results with the Infrared Optical Telescope Array Imaging Interferometer: Detection of Asymmetries in Asymptotic Giant Branch Stars

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Infrared and visual lunar occultations measurements of stellar diameters and new binary stars detections at the Calar Alto 1.5 m telescope

O. Fors, A. Richichi, J. Núñez and A. Prades
Astronomy & Astrophysics 419 (1) 285 (2004)
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Evidence of asymmetric structure in the atmosphere of Mira variable U Orionis from lunar occultation observations in the near-infrared

Soumen Mondal and T. Chandrasekhar
Monthly Notices of the Royal Astronomical Society 348 (4) 1332 (2004)
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