Influence of inelastic collisions with hydrogen atoms on the non-local thermodynamic equilibrium line formation for Fe I and Fe II in the 1D model atmospheres of late-type stars

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Table 2

LTE and NLTE abundances, log ε, from individual lines of Fe I and Fe II in HD 84937, HD 140283, and HD 122563.

λ,	E_exc,	log gf	HD 84937				HD 140283				HD 122563

Å	eV		W_obs	LTE	B18	YBK18	W_obs	LTE	B18	YBK18	W_obs	LTE	B18	YBK18
Fe I lines
4445.48	0.09	−5.44									14.6	4.82	4.97	4.94
4920.50	2.83	0.07	59.2	5.18	5.50	5.48	61.5	4.91	5.23	5.25	112.3	4.59	4.76	4.89
4994.13	0.92	−2.96	8.8	5.28	5.45	5.44	13.8	4.94	5.11	5.10	77.6	4.80	4.91	4.88

Notes. The two sets of the NLTE abundances correspond to different collisional recipes, namely, B18 and YBK18. Observed equivalent widths, W_obs, are given in mÅ. This table is available in its entirety at the CDS. A portion is shown here for guidance regarding its form and content.

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