The role of the hot porous layer in the gas flow in the inner coma

Open Access

Fig. 5

Spectral lines for a spherical nucleus. Comparison of the spectral lines for the 110–101 fundamental line transition for H₂¹⁶O at 556.937 GHz (left) and H₂¹⁸O at 547.676 GHz (right) at a 0° phase angle (a) and a 90° phase angle (b; terminator) for the different models.

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