Fig. 5
IRAS 07222−2005 (left panel) and IRAS 09194−4518 (right panel) display two components (circumstellar and photospheric) in the 7800 Å Rb I line (black line) and cannot be reproduced by our present version of the spectral synthesis code. The red line shows the pseudo-dynamical synthetic spectrum that gives a good fit to the photospheric component only.
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