Abridged Abstract - Utilizing the FORS2 instrument on the VLT, we have obtained near infrared spectra for more than 200 stars in 28 populous LMC clusters. This cluster sample spans a large range of ages (~ 1-13 Gyr) and metallicities (-0.3 > [Fe/H] > -2.0) and has good areal coverage of the LMC disk. The strong absorption lines of the Calcium II triplet are used to derive cluster radial velocities and abundances. We determine mean cluster velocities to typically 1.6 km/s and mean metallicities to 0.04 dex (random error). For eight of these clusters, we report the first spectroscopically determined metallicities based on individual cluster stars, and six of these eight have no published radial velocity measurements. (continued in paper
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
We present results obtained from spectroscopic observations of red giants located in the fields of t...
This paper represents a major step forward in the systematic and homogeneous study of Small Magellan...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
We report metallicities and radial velocities derived from spectra at the near-infrared calcium trip...
We report metallicities and radial velocities derived from spectra at the near-infrared calcium trip...
We obtained spectra of red giants in 15 Small Magellanic Cloud (SMC) clusters in the region of the C...
We aim to analyze the chemical evolution of the Small Magellanic Cloud adding 12 additional clusters...
We have obtained metallicities of ∼360 red giant stars distributed in 15 Small Magellanic Cloud (SMC...
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
We present results obtained from spectroscopic observations of red giants located in the fields of t...
This paper represents a major step forward in the systematic and homogeneous study of Small Magellan...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
Using the FORS2 instrument on the Very Large Telescope, we have obtained near-infrared spectra for m...
We report metallicities and radial velocities derived from spectra at the near-infrared calcium trip...
We report metallicities and radial velocities derived from spectra at the near-infrared calcium trip...
We obtained spectra of red giants in 15 Small Magellanic Cloud (SMC) clusters in the region of the C...
We aim to analyze the chemical evolution of the Small Magellanic Cloud adding 12 additional clusters...
We have obtained metallicities of ∼360 red giant stars distributed in 15 Small Magellanic Cloud (SMC...
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
Aims. In this paper we analyze the chemical evolution of the main body of the SMC, adding six additi...
We present results obtained from spectroscopic observations of red giants located in the fields of t...
This paper represents a major step forward in the systematic and homogeneous study of Small Magellan...