The nearby dwarf starburst galaxy NGC 5253 hosts a number of young, massive star clusters, the two youngest of which are centrally concentrated and surrounded...
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PublicationThe Brightest Young Star Clusters in NGC 5253.
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PublicationThe central region of M83: massive star formation, kinematics, and the location and origin of the nucleus
We report new near-IR integral field spectroscopy of the central starburst region of the barred spiral galaxy M83 obtained with Cambridge Infra-Red Panoramic...
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PublicationThe contribution to population in ellipticals of blue stragglers - A test of their origin
An observational test of the binary hypothesis for the origin of the blue straggler (BS) stars has been performed searching for radial velocity variables among...
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PublicationThe embedded cluster IRAS17136 - 3617 associated with the nebulosity GM24
Radio, infrared, and optical observations of the embedded infrared cluster IRAS17136 - 3617 are reviewed. The cluster consists of more than 25 stars with a...
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PublicationThe First Billion Years project: Finding infant globular clusters at z = 6
Aims: We aim to conduct an assessment of the demographics of substructures in cosmological simulations to identify low-mass stellar systems at high redshift...
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PublicationThe formation of super-star clusters in disk and dwarf galaxies
Super-star clusters are probably the largest star-forming entities in our local Universe, containing hundreds of thousands to millions of young stars usually...
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PublicationThe Fornax 3D project: Globular clusters tracing kinematics and metallicities
Globular clusters (GCs) are found ubiquitously in massive galaxies and due to their old ages, they are regarded as fossil records of galaxy evolution...
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PublicationThe Fornax 3D project: Non-linear colour-metallicity relation of globular clusters
Globular cluster (GC) systems of massive galaxies often show a bimodal colour distribution. This has been interpreted as a metallicity bimodality, created by a...
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PublicationThe Gaia-ESO Survey: chemical signatures of rocky accretion in a young solar-type star
It is well known that newly formed planetary systems undergo processes of orbital reconfiguration and planetary migration. As a result, planets or...