Variation of Silicate Dust Features with Phase Mid-IR Monitoring of Oxygen-Rich Mira Variable Stars

Details Variation of Silicate Dust Features with Phase Mid-IR Monitoring of Oxygen-Rich Mira Variable Stars Variation of Silicate Dust Features with Phase Mid-IR Monitoring of Oxygen-Rich Mira Variable Stars

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.251..157c&link_type=abstract

Astrophysics and Space Science, Volume 251, Issue 1-2, pp. 157-163

Astronomy and Astrophysics

Astrophysics

Scientific paper

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.

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