The multiple-shell model of circumstellar envelope of Mira variable.

Details The multiple-shell model of circumstellar envelope of Mira variable. The multiple-shell model of circumstellar envelope of Mira variable.

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993chsbu..38..216y&link_type=abstract

Chin. Sci. Bull., Vol. 38, No. 3, p. 216 - 220

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Scientific paper

It is shown from the author's computational results that the distribution of CO (2-1) molecules in the circumstellar envelope of a Mira variable has the structure of multiple shells. Considering the statistic fitting results for the distribution figure of the characteristic velocity region of the OH 1612 MHz maser obtained by VLBI, and analysis of the distinct phenomena of P Cyg-type spectra of the absorption line of gas molecules, the author concludes that the expanding multiple-shell model is the general proper model of the circumstellar envelope of a Mira variable.

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