Galactic chemical evolution of sulphur - Sulphur abundances from the [S i] λ1082 nm line in giants

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Table 3

Stellar parameters derived in this and previous works.

HD/BD	This study									Literature data
	T _eff	ΔT_eff	log g	Δlog g	[Fe/H]	Δ [Fe/H]	i	ξ	[(Fe+Cr)/H]	T _eff	log g	[Fe/H]


2796	5002	30	1.73	0.20	(−2.33)	0.13	...	1.8	...	4932	1.40	−2.33
3546	4977	30	2.44	0.12	−0.54	0.04	1, 2	1.4	−0.64	4923	2.48	−0.63
8724	4790	30	1.66	0.12	−1.55	0.07	1	1.8	...	4574	1.35	−1.75
10380	4216	30	1.48	0.08	−0.23	0.06	1	1.4	−0.20	4121	1.72	−0.27
13979	5052	159	(1.50)	0.49	(−2.57)	0.24	...	1.9	...	5043	1.50	−2.57
21581	5051	30	2.37	0.14	−1.50	0.04	1, 6, 7	1.6	...	4893	2.09	−1.70
23798	4482	33	0.71	0.12	−2.10	0.07	1, 5, 6, 7	2.1	...	4442	0.79	−2.12
26297	4484	30	0.83	0.10	−1.72	0.04	1, 3, 5, 6	2.0	...	4432	1.13	−1.75
29574	4299	30	0.51	0.34	−1.97	0.06	1, 3, 5, 6	2.1	...	4154	0.04	−1.93
34334	4308	30	1.87	0.06	−0.40	0.05	1, 3, 4	1.4	−0.36	4194	2.17	−0.37
36702	4337	30	(0.88)	0.10	−2.12	0.07	1, 3	2.0	...	4394	0.88	−2.03
37160	4771	30	2.57	0.05	−0.59	0.06	1, 3	1.3	−0.56	4729	2.65	−0.47
40460	4724	45	2.42	0.08	−0.21	0.05	1	1.2	−0.29	4541	2.00	−0.50
44007	4907	30	2.36	0.07	−1.67	0.06	1, 3, 6	1.6	...	4862	2.10	−1.64
65953	4038	30	1.19	0.07	−0.30	0.07	1	1.5	−0.28	3960	1.68	−0.36
81192	4779	30	2.46	0.04	−0.71	0.04	1, 2	1.4	−0.74	4728	2.58	−0.64
83212	4616	30	1.26	0.10	−1.44	0.04	1, 5, 6	1.8	...	4518	1.38	−1.45
85773	4443	30	1.00	0.12	(−2.24)	0.24	...	2.0	...	4431	0.91	−2.24
103545	5085	60	(1.70)	0.30	−1.70	0.08	1	1.8	...	4708	1.70	−2.14
110184	4374	30	(0.65)	0.40	−2.33	0.10	1	2.1	...	4342	0.65	−2.33
111721	5078	30	2.56	0.17	−1.30	0.07	1	1.5	...	5038	2.70	−1.34
117876	4772	30	2.35	0.10	−0.44	0.04	1, 2	1.3	−0.41	4722	2.27	−0.49
122563	4719	30	1.32	0.04	(−2.65)	0.16	...	1.9	...	4594	1.25	−2.65
122956	4698	37	1.44	0.11	−1.74	0.07	1	1.8	...	4618	1.50	−1.74
139195	4994	66	2.85	0.05	0.00	0.05	1, 2	1.1	−0.04	4991	3.03	−0.11
161074	3949	30	1.45	0.07	−0.03	0.09	1	1.3	−0.05	3997	1.83	−0.27
166161	5195	38	2.52	0.13	−1.18	0.07	1	1.5	...	5177	2.23	−1.21
168723	4936	30	3.04	0.03	−0.22	0.04	1	1.1	−0.21	4902	3.09	−0.14
184406	4530	30	2.70	0.06	0.20	0.04	1	1.0	0.18	4486	2.47	−0.04
187111	4418	30	0.70	0.11	−1.78	0.04	1, 3	2.1	...	4280	0.76	−1.75
188512	5111	79	3.52	0.06	−0.23	0.06	1, 2	1.2	−0.21	5107	3.56	−0.16
204543	4490	30	(1.25)	0.30	−1.97	0.07	1	1.9	...	4682	1.25	−1.82
212943	4694	30	2.61	0.06	−0.26	0.04	1, 2	1.2	−0.25	4611	2.79	−0.29
214567	4907	103	2.57	0.14	−0.19	0.08	1, 2	1.2	−0.20	5003	2.50	−0.03
216143	4362	113	(1.05)	0.49	−2.22	0.14	1	2.0	...	4511	1.05	−2.22
219615	4843	30	2.39	0.08	−0.56	0.04	1	1.4	−0.53	4848	2.52	−0.49
220954	4766	51	2.70	0.10	0.25	0.05	1	1.0	0.20	4708	2.74	−0.03
221170	4591	32	1.05	0.10	−2.00	0.07	1	2.0	...	4480	0.98	−2.11
+30 2611	4322	30	(0.90)	0.33	−1.43	0.07	1	1.9	−1.41	4291	0.90	−1.40

Notes. The quantities in parentheses denote log g and [Fe/H] values that were adopted from the literature (see the last two columns). i denotes the Fe i lines used in metallicity determination (ordered according to wavelength as in Table 2). Δξ is about 0.2–0.3 km s^-1. Literature data are the interquartile mean values taken from Soubiran et al. (2010).

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