Academia Sinica Institute of Astronomy & Astrophysics
中央研究院天文及天文物理研究所
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Interstellar and Circumstellar Medium

Schematic chemical structure of the circumstellar shell of an AGB star
Image Credit: Kemper, Francisca
Schematic chemical structure of the circumstellar shell of an AGB star
The top half of the plot represents the chemistry in an oxygen-rich environment (C/O < 1), and the bottom half of the figure shows the carbon-rich counterpart.
The logarithmic scale at the bottom shows the distance and temperature to the center of the star. Several distinct zones can be identified, namely the molecular formation region and the dust formation region, where conditions are governed by the density and the stellar radiation field, and the outermost region where the chemistry is dominated by the impinging interstellar radiation.
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