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Cracking the Relation between Mass and 1P Star Fraction of Globular Clusters. I. Present-day Cluster Masses as a First Tool

The Astrophysical journal, 2024-04, Vol.964 (2), p.140

Parmentier, Geneviève

2024

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Molecular Clumps Disguising Their Star Formation Efficiency per Free-fall Time: What We Can Do Not to Be Fooled

The Astrophysical journal, 2020-04, Vol.893 (1), p.32

Parmentier, Geneviève

2020

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The Long-term Evolution of Star Clusters Formed with a Centrally Peaked Star Formation Efficiency Profile

The Astrophysical journal, 2018-08, Vol.863 (2), p.171

2018

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From the molecular-cloud- to the embedded-cluster-mass function with a density threshold for star formation

Monthly notices of the Royal Astronomical Society, 2011-05, Vol.413 (3), p.1899-1912

Parmentier, Geneviève

2011

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Evidence for two populations of Galactic globular clusters from the ratio of their half-mass to Jacobi radii

Monthly notices of the Royal Astronomical Society, 2010-01, Vol.401 (3), p.1832-1838

2010

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The mass function and dynamical mass of young star clusters: why their initial crossing-time matters crucially

Monthly notices of the Royal Astronomical Society, 2012-12, Vol.427 (3), p.1940-1952

2012

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The origin of the Gaussian initial mass function of old globular cluster systems

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (1), p.352-372

2007

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The puzzle of the cluster-forming core mass-radius relation and why it matters

Monthly notices of the Royal Astronomical Society, 2011-02, Vol.411 (2), p.1258-1270

2011

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The poorly constrained cluster disruption time-scale in the Large Magellanic Cloud

Monthly notices of the Royal Astronomical Society, 2008-01, Vol.383 (3), p.1103-1120

2008

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Volume density thresholds for overall star formation imply mass-size thresholds for massive star formation

Monthly notices of the Royal Astronomical Society, 2011-09, Vol.416 (1), p.783-789

2011

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New light on the initial mass function of the Galactic halo globular clusters

Monthly notices of the Royal Astronomical Society, 2005-10, Vol.363 (1), p.326-336

2005

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Star Clusters in the Galactic tidal field, from birth to dissolution

Proceedings of the International Astronomical Union, 2019-05, Vol.14 (S351), p.507-511

2019

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Early dynamical evolution of star cluster systems

Proceedings of the International Astronomical Union, 2009-08, Vol.5 (S266), p.87-94

Parmentier, Geneviève

2009

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From the molecular-cloud- to the embedded-cluster-mass function with a density threshold for star formation: Cloud and cluster mass functions

Monthly notices of the Royal Astronomical Society, 2011-05, Vol.413 (3), p.1899-1912

Parmentier, Geneviève

2011

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Gas removal and the initial mass function of star clusters

Astrophysics and space science, 2009-12, Vol.324 (2-4), p.327-332

2009

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On the origin of the radial mass density profile of the Galactic halo globular cluster system

Monthly notices of the Royal Astronomical Society, 2005-05, Vol.359 (2), p.615-623

2005

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The mass function and dynamical mass of young star clusters: why their initial crossing-time matters crucially: Star cluster early evolutionary rates

Monthly notices of the Royal Astronomical Society, 2012-12, Vol.427 (3), p.1940-1952

2012

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The puzzle of the cluster-forming core mass-radius relation and why it matters: Cluster-forming core mass-radius relation

Monthly notices of the Royal Astronomical Society, 2011-02, Vol.411 (2), p.1258-1270

2011

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Self-enrichment of Galactic halo globular clusters: stimulated star formation and consequences for the halo metallicity distribution

Monthly notices of the Royal Astronomical Society, 2004-06, Vol.351 (2), p.585-598

Parmentier, Geneviève

2004

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The Long-term Survival Chances of Young Massive Star Clusters

Chinese journal of astronomy and astrophysics, 2007-04, Vol.7 (2), p.155-186

2007

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Self-enrichment of Galactic halo globular clusters: stimulated star formation and consequences for the halo metallicity distribution

Monthly notices of the Royal Astronomical Society, 2004-06, Vol.351 (2), p.585-598

Parmentier, Geneviève

2004

Volltextzugriff (PDF)

The origin of the Gaussian initial mass function of old globular cluster systems

Monthly notices of the Royal Astronomical Society, 2007-05, Vol.377 (1), p.352-372

2007

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The poorly constrained cluster disruption time-scale in the Large Magellanic Cloud

Monthly notices of the Royal Astronomical Society, 2008-01, Vol.383 (3), p.1103-1120

2008

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The poorly constrained cluster disruption time-scale in the Large Magellanic Cloud: The LMC star cluster system

Monthly notices of the Royal Astronomical Society, 2008-01, Vol.383 (3), p.1103-1120

2008

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Volume density thresholds for overall star formation imply mass-size thresholds for massive star formation: Massive star formation mass-size thresholds

Monthly notices of the Royal Astronomical Society, 2011-06, p.no-no

2011

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Cracking the Relation between Mass and 1P Star Fraction of Globular Clusters. I. Present-day Cluster Masses as a First Tool

Molecular Clumps Disguising Their Star Formation Efficiency per Free-fall Time: What We Can Do Not to Be Fooled

The Long-term Evolution of Star Clusters Formed with a Centrally Peaked Star Formation Efficiency Profile

From the molecular-cloud- to the embedded-cluster-mass function with a density threshold for star formation

Evidence for two populations of Galactic globular clusters from the ratio of their half-mass to Jacobi radii

The mass function and dynamical mass of young star clusters: why their initial crossing-time matters crucially

The origin of the Gaussian initial mass function of old globular cluster systems

The puzzle of the cluster-forming core mass-radius relation and why it matters

The poorly constrained cluster disruption time-scale in the Large Magellanic Cloud

Volume density thresholds for overall star formation imply mass-size thresholds for massive star formation

New light on the initial mass function of the Galactic halo globular clusters

Star Clusters in the Galactic tidal field, from birth to dissolution

Early dynamical evolution of star cluster systems

From the molecular-cloud- to the embedded-cluster-mass function with a density threshold for star formation: Cloud and cluster mass functions

Gas removal and the initial mass function of star clusters

On the origin of the radial mass density profile of the Galactic halo globular cluster system

The mass function and dynamical mass of young star clusters: why their initial crossing-time matters crucially: Star cluster early evolutionary rates

The puzzle of the cluster-forming core mass-radius relation and why it matters: Cluster-forming core mass-radius relation

Self-enrichment of Galactic halo globular clusters: stimulated star formation and consequences for the halo metallicity distribution

The Long-term Survival Chances of Young Massive Star Clusters

Self-enrichment of Galactic halo globular clusters: stimulated star formation and consequences for the halo metallicity distribution

The origin of the Gaussian initial mass function of old globular cluster systems

The poorly constrained cluster disruption time-scale in the Large Magellanic Cloud

The poorly constrained cluster disruption time-scale in the Large Magellanic Cloud: The LMC star cluster system

Volume density thresholds for overall star formation imply mass-size thresholds for massive star formation: Massive star formation mass-size thresholds

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