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20002026
most citedA Universal Stellar Initial Mass Function? A Critical Look at Variations

1k citations · 15.4k across the 253 of their papers we have counts for

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Showing 2017 · astro-ph.GAShow all

10 papers · 2 filters

astro-ph.GA2017★ 241 cited

The E-MOSAICS Project: simulating the formation and co-evolution of galaxies and their star cluster populations

Joel Pfeffer, J. M. Diederik Kruijssen, Robert A. Crain +1

We introduce the MOdelling Star cluster population Assembly In Cosmological Simulations within EAGLE (E-MOSAICS) project. E-MOSAICS incorporates models describing the formation, ev…

astro-ph.GA2017★ 1 cited

Interpreting the complex CMDs of the Magellanic Clouds clusters

I. Cabrera-Ziri, S. Martocchia, K. Hollyhead +1

The Magellanic Clouds host a large population of massive (> 10^4 Msun) star clusters with ages ranging from a few Myr to 12 Gyr. In nearly all cases, close inspection of their CMDs…

astro-ph.GA2017★ 136 cited

Nearby Early-Type Galactic Nuclei at High Resolution: Dynamical Black Hole and Nuclear Star Cluster Mass Measurements

Dieu D. Nguyen, Anil C. Seth, Nadine Neumayer +12

We present a detailed study of the nuclear star clusters (NSCs) and massive black holes (BHs) of four of the nearest low-mass early-type galaxies: M32, NGC205, NGC5012, and NGC5206…

astro-ph.GA2017★ 129 cited

Age as a Major Factor in the Onset of Multiple Populations in Stellar Clusters

S. Martocchia, I. Cabrera-Ziri, C. Lardo +16

It is now well established that globular clusters (GCs) exhibit star-to-star light-element abundance variations (known as multiple stellar populations, MPs). Such chemical anomalie…

astro-ph.GA2017★ 51 cited

Red Supergiants as Cosmic Abundance Probes: massive star clusters in M83, and the mass-metallicity relation of nearby galaxies

Ben Davies, Rolf-Peter Kudritzki, Carmela Lardo +6

We present an abundance analysis of seven super-star clusters in the disk of M83. The near-infrared spectra of these clusters are dominated by Red Supergiants, and the spectral sim…

astro-ph.GA2017★ 48 cited

The difference in metallicity distribution functions of halo stars and globular clusters as a function of galaxy type: A tracer of globular cluster formation and evolution

Henny J. G. L. M. Lamers, J. M. Diederik Kruijssen, Nate Bastian +3

Observations of globular clusters (GCs) and field stars in the halos of the giant elliptical galaxy Cen A and the spiral galaxy M31 show a large range of cluster-to-star number rat…

astro-ph.GA2017★ 68 cited

Thermal Feedback in the high-mass star and cluster forming region W51

Adam Ginsburg, Ciriaco Goddi, J. M. Diederik Kruijssen +11

High-mass stars have generally been assumed to accrete most of their mass while already contracted onto the main sequence, but this hypothesis has not been observationally tested.…

astro-ph.GA2017★ 70 cited

The Search for Multiple Populations in Magellanic Cloud Clusters III: No evidence for Multiple Populations in the SMC cluster NGC 419

S. Martocchia, N. Bastian, C. Usher +16

We present the third paper about our ongoing HST survey for the search for multiple stellar populations (MPs) within Magellanic Cloud clusters. We report here the analysis of NGC 4…

astro-ph.GA2017★ 18 cited

Searching for GC-like abundance patterns in young massive clusters II. - Results from the Antennae galaxies

C. Lardo, I. Cabrera-Ziri, B. Davies +1

The presence of multiple populations (MPs) with distinctive light element abundances is a widespread phenomenon in clusters older than 6 Gyr. Clusters with masses, luminosities, an…

astro-ph.GA2017★ 71 cited

The Varying Mass Distribution of Molecular Clouds Across M83

Pamela Freeman, Erik Rosolowsky, J. M. Diederik Kruijssen +2

The work of Adamo et al. (2015) showed that the mass distributions of young massive stellar clusters were truncated above a maximum-mass scale in the nearby galaxy M83 and that thi…