CO and HCN isotopologue ratios in the outflows of AGB stars

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Table 3

Model assumptions for reference models with different mass-loss rates used in the radiative transfer modeling.

R_⋆	L_⋆	T_⋆	V_exp	T_dust ⁽¹⁾	R_in
(cm)	(L_⊙)	(K)	(km s⁻¹)	(K)	(cm)
3.5 × 10¹³	9000	2500	15		1 × 10¹⁴

Notes. ⁽¹⁾ T_in is the dust condensation temperature and is assumed to be 1200 and 1500 K for C-type and O-type CSEs, respectively.

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