As part of our uninterrupted systematic study of star clusters in the Large Magellanic Cloud (LMC), we present preliminary results for 4 faint, unstudied LMC star clusters. Based on CCD images in the Washington system obtained with the 4 m telescope at Cerro Tololo Inter-American Observatory (Chile), we derive approximate ages and metallicities using theoretical isochrones in the (T,C-T1) diagrams. The clusters are aged between 550 and 1300 Myr, being all of them relatively metal-poor. Their approximate radii were estimated from stellar density profiles. The current study will be soon extended into a vast LMC region wherein numerous unstudied star clusters can be found (Palma 20...
Aims. The main goal of this study is to compile a catalogue of the fundamental parameters of a compl...
We present Eashington system colour-magnitude diagramsfor 8 stars clusters and their surrounding fie...
We present Eashington system colour-magnitude diagramsfor 8 stars clusters and their surrounding fie...
As part of our uninterrupted systematic study of star clusters in the Large Magellanic Cloud (LMC), ...
As part of our uninterrupted systematic study of star clusters in the Large Magellanic Cloud (LMC), ...
Based on CCD images obtained in the Washington system at Cerro Tololo Inter-American Observatory, we...
Based on CCD images obtained in the Washington system at Cerro Tololo Inter-American Observatory, we...
Using Washington photometry, we determine linear radii, ages and metallicities of NGC 2161, SL 874 a...
We present Washington system colour-magnitude diagrams (CMDs) for 17 practically unstudied star clus...
As part of an ongoing project to investigate the cluster formation and chemical evolution history in...
We present the results of 16 Large Magellanic Cloud (LMC) clusters obtained for the first time from ...
We present CCD photometry in the Washington system C and T1 bands of 14 star clusters of the Small M...
Aims. We present CCD photometry in the Washington system C and T1 passbands down to T1 ∼ 22.5 in the...
We present the results on the age estimates of 11 Small Magellanic Cloud (SMC) clusters obtained for...
Using Ca triplet spectroscopy and P SF photometry performed on data taken with the “Very Large Teles...
Aims. The main goal of this study is to compile a catalogue of the fundamental parameters of a compl...
We present Eashington system colour-magnitude diagramsfor 8 stars clusters and their surrounding fie...
We present Eashington system colour-magnitude diagramsfor 8 stars clusters and their surrounding fie...
As part of our uninterrupted systematic study of star clusters in the Large Magellanic Cloud (LMC), ...
As part of our uninterrupted systematic study of star clusters in the Large Magellanic Cloud (LMC), ...
Based on CCD images obtained in the Washington system at Cerro Tololo Inter-American Observatory, we...
Based on CCD images obtained in the Washington system at Cerro Tololo Inter-American Observatory, we...
Using Washington photometry, we determine linear radii, ages and metallicities of NGC 2161, SL 874 a...
We present Washington system colour-magnitude diagrams (CMDs) for 17 practically unstudied star clus...
As part of an ongoing project to investigate the cluster formation and chemical evolution history in...
We present the results of 16 Large Magellanic Cloud (LMC) clusters obtained for the first time from ...
We present CCD photometry in the Washington system C and T1 bands of 14 star clusters of the Small M...
Aims. We present CCD photometry in the Washington system C and T1 passbands down to T1 ∼ 22.5 in the...
We present the results on the age estimates of 11 Small Magellanic Cloud (SMC) clusters obtained for...
Using Ca triplet spectroscopy and P SF photometry performed on data taken with the “Very Large Teles...
Aims. The main goal of this study is to compile a catalogue of the fundamental parameters of a compl...
We present Eashington system colour-magnitude diagramsfor 8 stars clusters and their surrounding fie...
We present Eashington system colour-magnitude diagramsfor 8 stars clusters and their surrounding fie...