The chemical composition of a regular halo globular cluster: NGC 5897

Andreas Koch; Andrew McWilliam

doi:10.1051/0004-6361/201323119

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Volume 565 (May 2014)

A&A, 565 (2014) A23

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Table 1

Properties of the targeted stars.

ID^a	Alt. ID^b	α	δ	V	V − I	V − K	Date of obs.	t_exp	S/N^c	v_HC
ID^a	Alt. ID^b	(J2000.0)	(J2000.0)	[mag]	[mag]	[mag]	Date of obs.	[s]	[pixel^-1]	[km s^-1]

S-255	ESO-1702	15:17:30.07	−21:02:08.81	13.32	1.59	3.64	2013-May-10	6340	115	104.6
S-20^d	ESO-32	15:17:14.73	−20:56:57.18	13.34	1.58	3.59	2013-May-07	1800	110	100.1
S-9	ESO-3884	15:17:30.51	−20:56:58.90	13.51	1.54	3.51	2013-May-07	2160	120	100.9
S-366	ESO-6910	15:17:14.06	−21:04:19.72	13.95	1.38	3.10	2013-May-07	3600	105	101.8
S-138	ESO-4959	15:17:39.38	−20:59:53.25	14.48	1.27	3.06	2013-May-07, 08	8100	120	101.1
S-290	ESO-5660	15:17:09.41	−21:01:46.98	14.48	1.23	2.89	2013-May-10	6600	100	102.2
S-364	ESO-1974	15:17:21.49	−21:04:40.91	14.71	1.19	2.83	2013-May-11	5400	90	103.3

...	ESO-4678^e	15:17:45.47	−21:01:54.93	14.67	1.20	2.73	2013-May-10,11	5400	100	−52.7

Notes.

^(a)

Identifications from Sandage & Katem (1968).

^(b)

ID from Testa et al. (2001).

^(c)

Measured in the order containing Hα.

^(d)

Variable star ≡V-5 (Sandage & Katem 1968).

^(e)

Non-member.

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