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20022008
most citedThe nucleus of the Sagittarius dSph galaxy and M54: a window on the process of galaxy nucleation

230 citations · 932 across the 9 of their papers we have counts for

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11 papers · 1 filter

astro-ph200849 cited

On the origin of double main-sequence turn-offs in star clusters of the Magellanic Clouds

K. Bekki, A. D. Mackey

Recent observational studies of intermediate-age star clusters (SCs) in the Large Magellanic Cloud (LMC) have reported that a significant number of these objects show double main-s…

astro-ph2008230 cited

The nucleus of the Sagittarius dSph galaxy and M54: a window on the process of galaxy nucleation

M. Bellazzini, R. A. Ibata, S. C. Chapman +6

We present the results of a thorough study of the nucleus of the Sgr dwarf spheroidal galaxy and of the bright globular cluster M54 that resides within the same nucleus (Sgr,N). We…

astro-ph2008178 cited

Multiple stellar populations in three rich Large Magellanic Cloud star clusters

A. D. Mackey, P. Broby Nielsen, A. M. N. Ferguson +1

We present deep colour-magnitude diagrams for three rich intermediate-age star clusters in the Large Magellanic Cloud, constructed from archival ACS F435W and F814W imaging. All th…

astro-ph200714 cited

Simple Stellar Population Models as probed by the Large Magellanic Cloud Star Cluster ESO 121-SC03

Y. Xin, L. Deng, R. de Grijs +2

The presence of blue straggler stars (BSs) in star clusters has proven a challenge to conventional simple stellar population (SSP) models. Conventional SSP models are based on the…

astro-ph2007207 cited

A double main sequence turn-off in the rich star cluster NGC 1846 in the Large Magellanic Cloud

A. D. Mackey, P. Broby Nielsen

We report on HST/ACS photometry of the rich intermediate-age star cluster NGC 1846 in the Large Magellanic Cloud, which clearly reveals the presence of a double main sequence turn-…

astro-ph200795 cited

The effect of stellar-mass black holes on the structural evolution of massive star clusters

A. D. Mackey, M. I. Wilkinson, M. B. Davies +1

We present the results of realistic N-body modelling of massive star clusters in the Magellanic Clouds, aimed at investigating a dynamical origin for the radius-age trend observed…