Mid-IR Observations of Mira Circumstellar Environment

Abstract

This paper presents results from high-angular resolution mid-IR imaging of the Mira AB circumbinary environment using the MIRAC3 camera at the NASA Infrared Telescope Facility (IRTF). We resolved the dusty circumstellar envelope at 9.8, 11.7 and 18 micron around Mira A (o Ceti), and measured the size of the extended emission. Strong deviations from spherical symmetry are detected in the images of Mira AB system, including possible dust clumps in the direction of the companion (Mira B). These observations suggest that Mira B plays an active role in shaping the morphology of the circumstellar environment of Mira A as it evolves toward the Planetary Nebula phase.

11 pages, 2 PostScript figures, accepted for publication in the Astrophysical Journal Letters

References in corpus (1)

• 100-year Mass Loss Modulations on the Asymptotic Giant Branch

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• A Phenomenological Model for the Extended Zone Above AGB Stars
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