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Variation of Silicate Dust Features with Phase Mid-IR Monitoring of Oxygen-Rich Mira Variable Stars
Authors:Michelle J Creech-Eakman  Robert E Stencel
Institution:(1) Dept. of Physics and Astronomy, University of Denver, Denver, CO, USA
Abstract:We present photometric and spectroscopic data on a subset of over 30 oxygen-rich Long Period Variable (LPV) stars which we have been monitoring between 8/95 & 4/97. With these data, we are attempting to ascertain the relationship of dust formation to optical period. Our ultimate goal is to determine what conditions lead to dust formation and destruction in these environments, and whether or not an evolutionary sequence can be inferred for AGB stars also based on their spectra and dust formation. This revised version was published online in September 2006 with corrections to the Cover Date.
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