Add to ORKGWe present colour-magnitude diagrams for two rich (~~104 M̛) Large Magellanic Cloud star clusters with ages ~~ 107 yr, constructed from optical and near-infrared data obtained with the Hubble Space Telescope. These data are part of an HST project to study LMC clusters with a range of ages. In this paper we investigate the massive star content of the young clusters, and determine the cluster ages and metallicities, paying particular attention to Be-star and blue-straggler populations and evidence of age spreads. We compare our data with detailed stellar-population simulations to investigate the turn-off structure of ~~ 25 Myr stellar systems, highlighting the complexity of the blue-straggler phenomenon
The optical integrated spectra of three Large Magellanic Cloud young stellar clusters (NGC 1984, NGC...
In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Mage...
Aims. We study 147 star clusters in the Large Magellanic Cloud (LMC) in order to determine their mea...
We present colour-magnitude diagrams for two rich (~~104 M̛) Large Magellanic Cloud star clusters wi...
We present Washington System photometry for 11 star clusters immersed in the north-west part of the ...
Using a combination of high-resolution Hubble Space Telescope/Wide-Field and Planetary Camera-2 obse...
Using a combination of high-resolution Hubble Space Telescope/Wide-Field and Planetary Camera-2 obse...
Recent discoveries have put the picture of stellar clusters being simple stellar populations into qu...
Using a combination of high-resolution Hubble Space Telescope/WFPC2 ob-servations, we explore the ph...
We show the results of deep V and I HST photometry of 6 rich star clusters in the Large Magellanic C...
Aims. In this paper we discuss the age and spatial distribution of young (age < 1 Gyr) Small Magella...
We show the results of deep V and I HST photometry of 6 rich star clusters in the Large Magellanic ...
Aims. In this paper we discuss the age and spatial distribution of young (age < 1 Gyr) Small Magella...
Young and intermediate-age star clusters of both Magellanic Clouds exhibit complex colour-magnitude ...
Aims. Integrated spectroscopy of a sample of 17 blue concentrated Large Magellanic Cloud (LMC) clust...
The optical integrated spectra of three Large Magellanic Cloud young stellar clusters (NGC 1984, NGC...
In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Mage...
Aims. We study 147 star clusters in the Large Magellanic Cloud (LMC) in order to determine their mea...
We present colour-magnitude diagrams for two rich (~~104 M̛) Large Magellanic Cloud star clusters wi...
We present Washington System photometry for 11 star clusters immersed in the north-west part of the ...
Using a combination of high-resolution Hubble Space Telescope/Wide-Field and Planetary Camera-2 obse...
Using a combination of high-resolution Hubble Space Telescope/Wide-Field and Planetary Camera-2 obse...
Recent discoveries have put the picture of stellar clusters being simple stellar populations into qu...
Using a combination of high-resolution Hubble Space Telescope/WFPC2 ob-servations, we explore the ph...
We show the results of deep V and I HST photometry of 6 rich star clusters in the Large Magellanic C...
Aims. In this paper we discuss the age and spatial distribution of young (age < 1 Gyr) Small Magella...
We show the results of deep V and I HST photometry of 6 rich star clusters in the Large Magellanic ...
Aims. In this paper we discuss the age and spatial distribution of young (age < 1 Gyr) Small Magella...
Young and intermediate-age star clusters of both Magellanic Clouds exhibit complex colour-magnitude ...
Aims. Integrated spectroscopy of a sample of 17 blue concentrated Large Magellanic Cloud (LMC) clust...
The optical integrated spectra of three Large Magellanic Cloud young stellar clusters (NGC 1984, NGC...
In our HST photometric survey, we have been searching for multiple stellar populations (MPs) in Mage...
Aims. We study 147 star clusters in the Large Magellanic Cloud (LMC) in order to determine their mea...