2000A&A...364L..19H

Query : 2000A&A...364L..19H

2000A&A...364L..19H - Astronomy and Astrophysics, volume 364L19-25 (2000/12-1)

Age-metallicity relation and chemical evolution of the LMC from UVES spectra of Globular Cluster giants.

HILL V., FRANCOIS P., SPITE M., PRIMAS F. and SPITE F.

Abstract (from CDS):

We report on the first high-resolution spectroscopy of 10 giants in LMC Globular Clusters in a wide age range, obtained with the newly commissioned spectrograph UVES at VLT UT2. These observations are used to derive oxygen and iron content of these clusters, and the abundances are then used to cast a more precise view, not only on the age-metallicity relation in the LMC, but also on the chemical evolution of this dwarf irregular galaxy.

Abstract Copyright: ∼

Journal keyword(s): stars: binaries: spectroscopic - stars: late-type - Galaxy: globular clusters: individual: NGC 2210, ESO 121-SCO3, NGC 1978, NGC 1866 - galaxies: Magellanic Clouds

CDS comments: Table 2: stars 4364, 110, 4793 in NGC 2210 not identified.

Simbad objects: 13

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Number of rows : 13
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 NAME SMC G 00 52 38.0 -72 48 01   2.79 2.2     ~ 12317 1
2 NGC 1866 GlC 05 13 38.920 -65 27 52.75           ~ 437 0
3 2MASS J05134025-6527197 LP* 05 13 40.2456742488 -65 27 19.581030756   16.50 15.01     ~ 9 0
4 Cl* NGC 1866 W 3974 * 05 13 46.3058794680 -65 27 10.278438516   17.017 15.49     ~ 10 0
5 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 19090 0
6 NGC 1978 GlC 05 28 45.330 -66 14 12.04   10.7 10.70     ~ 317 0
7 2MASS J05284847-6614387 LP* 05 28 48.4773620424 -66 14 38.660230788   18.375   15.25 14.50 MIII 16 0
8 Cl* NGC 1978 LE 9 * 05 28 50.7437780832 -66 14 44.111813712       16.33 14.69 M1 19 0
9 ESO 121-3 Cl* 06 02 03.32 -60 31 25.6   14.91 14.04     ~ 118 0
10 NGC 2210 GlC 06 11 31.296 -69 07 17.04   10.9 10.94     ~ 196 0
11 Cl* NGC 1866 BBC 867 * ~ ~   17.74 16.60     ~ 4 0
12 [MHS86] 313 * ~ ~           ~ 3 0
13 [MHS86] 167 * ~ ~           ~ 2 0

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