939 citations · 1.9k across the 33 of their papers we have counts for
33 papers
Cracking the relation between mass and 1P-star fraction of globular clusters: I. Present-day cluster masses as a first tool
Geneviève Parmentier
The phenomenon of multiple stellar populations is exacerbated in massive globular clusters, with the fraction of first-population (1P) stars a decreasing function of the cluster pr…
Rebounding Cores to Build Star Cluster Multiple Populations
G. Parmentier, A. Pasquali
We present a novel approach to the riddle of star cluster multiple populations. Stars form from molecular cores. But not all cores form stars. Following their initial compression,…
A new parameterization of the star formation rate-dense gas mass relation: embracing gas density gradients
G. Parmentier, A. Pasquali
It is well-established that a gas density gradient inside molecular clouds and clumps raises their star formation rate compared to what they would experience from a gas reservoir o…
Molecular clumps disguising their star formation efficiency per freefall time: What we can do not to be fooled
Genevieve Parmentier
The presence of a volume density gradient in molecular clumps allow them to raise their star formation rate compared to what they would experience were their gas uniform in density…
The density gradient inside molecular-gas clumps as a booster of their star formation activity
Genevieve Parmentier
Star-forming regions presenting a density gradient experience a higher star formation rate than if they were of uniform density. We refer to the ratio between the star formation ra…
Star Clusters in the Galactic tidal field, from birth to dissolution
Bekdaulet Shukirgaliyev, Genevieve Parmentier, Peter Berczik +1
We study the evolution of star clusters in the Galactic tidal field starting from their birth in molecular clumps. Our model clusters form according to the local-density-driven clu…