We present the results on the age estimates of 36 Large Magellanic Cloud (LMC) clusters obtained for the first time from CCD Washington CT1T2 photometry. By using the (T1, C − T1) and (T1, T1 − T2) diagrams, we estimated ages for the cluster sample using the δT1 index. We confirm that the studied cluster sample belong to the ∼ 2 Gyr bursting formation epoch of the LMC. Furthermore, when rebuiling the cluster age distribution -taken into account the estimated age errorswe found that the number of clusters with ages between 1-3 Gyr now doubles that of the known bursting cluster population, which suggests that the tidal interaction between both Magellanic Clouds and, perhaps, also the Milky Way, was more stronger than expected. A detail...
Integrated spectra in the range (3600-6800) A for a sample of 17 blue concentrated Large Magellanic...
We have used Washington photometry for 90 star cluster candidates of small angular size – typically ...
We report results on star clusters located in the South-Eastern half of the Large Magellanic (LMC) b...
We present the results on the age estimates of 36 Large Magellanic Cloud (LMC) clusters obtained for...
We present the results on the age estimates of 36 Large Magellanic Cloud (LMC) clusters obtained for...
Colour–magnitude diagrams (CMDs) are presented for the first time for 10 star clusters projected on ...
We present the results of 16 Large Magellanic Cloud (LMC) clusters obtained for the first time from ...
Using Washington photometry, we determine linear radii, ages and metallicities of NGC 2161, SL 874 a...
Aims. The main goal of this study is to compile a catalogue of the fundamental parameters of a compl...
We present our new, fully automated method to detect and measure the ages of star clusters in nearby...
As part of an ongoing project to investigate the cluster formation and chemical evolution history in...
We present CCD photometry in the Washington system C and T1 bands of 14 star clusters of the Small M...
We present the results on the age estimates of 11 Small Magellanic Cloud (SMC) clusters obtained for...
We analysed Washington CMT1 photometry of star clusters located along the minor axis of the Large Ma...
We analysed Washington CMT1 photometry of star clusters located along the minor axis of the Large Ma...
Integrated spectra in the range (3600-6800) A for a sample of 17 blue concentrated Large Magellanic...
We have used Washington photometry for 90 star cluster candidates of small angular size – typically ...
We report results on star clusters located in the South-Eastern half of the Large Magellanic (LMC) b...
We present the results on the age estimates of 36 Large Magellanic Cloud (LMC) clusters obtained for...
We present the results on the age estimates of 36 Large Magellanic Cloud (LMC) clusters obtained for...
Colour–magnitude diagrams (CMDs) are presented for the first time for 10 star clusters projected on ...
We present the results of 16 Large Magellanic Cloud (LMC) clusters obtained for the first time from ...
Using Washington photometry, we determine linear radii, ages and metallicities of NGC 2161, SL 874 a...
Aims. The main goal of this study is to compile a catalogue of the fundamental parameters of a compl...
We present our new, fully automated method to detect and measure the ages of star clusters in nearby...
As part of an ongoing project to investigate the cluster formation and chemical evolution history in...
We present CCD photometry in the Washington system C and T1 bands of 14 star clusters of the Small M...
We present the results on the age estimates of 11 Small Magellanic Cloud (SMC) clusters obtained for...
We analysed Washington CMT1 photometry of star clusters located along the minor axis of the Large Ma...
We analysed Washington CMT1 photometry of star clusters located along the minor axis of the Large Ma...
Integrated spectra in the range (3600-6800) A for a sample of 17 blue concentrated Large Magellanic...
We have used Washington photometry for 90 star cluster candidates of small angular size – typically ...
We report results on star clusters located in the South-Eastern half of the Large Magellanic (LMC) b...