We use the angular two-point correlation function (TPCF) to investigate the hierarchical distribution of young star clusters in 12 local (3-18 Mpc) star-forming galaxies using star cluster catalogs obtained with the Hubble Space Telescope (HST) as part of the Treasury Program Legacy ExtraGalactic UV Survey. The sample spans a range of different morphological types, allowing us to infer how the physical properties of the galaxy affect the spatial distribution of the clusters. We also prepare a range of physically motivated toy models to compare with and interpret the observed features in the TPCFs. We find that, conforming to earlier studies, young clusters ($T \lesssim 10\, \mathrm{Myr}$) have power-law TPCFs that are characteristic of frac...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
International audienceIn the hierarchical view of star formation, giant molecular clouds (GMCs) unde...
We present a study of the spatial distribution of the stellar cluster populations in the star-formin...
We present a study of the hierarchical clustering of the young stellar clusters in six local (3-15 M...
Aims. We study the connection between spatially resolved star formation and young star clusters acr...
We present an analysis of the positions and ages of young star clusters in eight local galaxies to i...
We present a study of the hierarchical clustering of the young stellar clusters in six local (3–15 M...
Aims. We study the connection between spatially resolved star formation and young star clusters acro...
Young stellar groupings and clusters have hierarchical patterns ranging from flocculent spiral arms ...
International audienceWe present a study of the spatial distribution of the stellar cluster populati...
Star clusters form the basic building blocks of galaxies. They span a wide range of ages, from a few...
Some years ago we proposed a new approach to the analysis of galaxy and cluster correlations based o...
Some years ago we proposed a new approach to the analysis of galaxy and cluster correlations based o...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
International audienceIn the hierarchical view of star formation, giant molecular clouds (GMCs) unde...
We present a study of the spatial distribution of the stellar cluster populations in the star-formin...
We present a study of the hierarchical clustering of the young stellar clusters in six local (3-15 M...
Aims. We study the connection between spatially resolved star formation and young star clusters acr...
We present an analysis of the positions and ages of young star clusters in eight local galaxies to i...
We present a study of the hierarchical clustering of the young stellar clusters in six local (3–15 M...
Aims. We study the connection between spatially resolved star formation and young star clusters acro...
Young stellar groupings and clusters have hierarchical patterns ranging from flocculent spiral arms ...
International audienceWe present a study of the spatial distribution of the stellar cluster populati...
Star clusters form the basic building blocks of galaxies. They span a wide range of ages, from a few...
Some years ago we proposed a new approach to the analysis of galaxy and cluster correlations based o...
Some years ago we proposed a new approach to the analysis of galaxy and cluster correlations based o...
We discuss some of the basic implications of recent results on galaxy correlations published by the ...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
We use the Two-Degree Field Galaxy Redshift Survey (2dFGRS) to test the hierarchical scaling hypothe...
International audienceIn the hierarchical view of star formation, giant molecular clouds (GMCs) unde...
We present a study of the spatial distribution of the stellar cluster populations in the star-formin...