The Gaia-ESO Survey: Detailed abundances in the metal-poor globular cluster NGC 4372

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Volume 579 (July 2015)

A&A, 579 (2015) A6

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Table 1

Basic parameters of the observed stars.

	Cname^a	v _rad	SNR ^b	T _eff	log(g)	ξ	[Fe/H]
		(km s^-1)		(K)	(dex)	(km s^-1)	(dex)


1	12250638-7243067	68.6 ± 0.5	51.17	4586 ± 86	0.70 ± 0.20	1.56 ± 0.10	–2.23 ± 0.21
2	12250660-7239224	67.9 ± 0.3	34.63	4646 ± 56	1.17 ± 0.15	1.68 ± 0.03	–2.22 ± 0.15
3	12253419-7235252	72.7 ± 0.7	55.73	4527 ± 33	0.55 ± 0.07	1.50 ± 0.17	–2.15 ± 0.07
4	12253882-7245095	76.0 ± 0.6	45.45	4656 ± 114	1.19 ± 0.47	1.56 ± 0.20	–2.21 ± 0.20
5	12260765-7236514	75.2 ± 0.5	71.14	4466 ± 38	0.55 ± 0.09	1.65 ± 0.05	–2.20 ± 0.17
6	12264293-7241576	71.0 ± 0.7	44.35	4712 ± 87	1.19 ± 0.21	1.55 ± 0.13	–2.15 ± 0.12
7	12264875-7239413	76.9 ± 0.4	43.89	4633 ± 68	0.84 ± 0.34	1.54 ± 0.05	–2.44 ± 0.16

Notes.

^(a)

GES object name. It is formed from the coordinates of the object splicing the RA in hours, minutes, and seconds (to 2 decimal places) and the Dec in degrees, minutes, and seconds (to 1 decimal place) together, including a sign for the declination.

^(b)

Mean signal-to-noise ratio in the spectrum.

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