Ruprecht-Karls-Universität Heidelberg

Dr. Geneviève Parmentier, Priv.-Doz.

Astronomisches Rechen-Institut



Office
Neubau, Room N.2-21

Postal Address
Zentrum für Astronomie der Universität Heidelberg
Astronomisches Rechen-Institut
Mönchhofstr. 12-14
69120 Heidelberg






12.
4/2024
Parmentier, Geneviève
Cracking the Relation between Mass and 1P Star Fraction of Globular Clusters. I. Present-day Cluster Masses as a First Tool
ApJ 964, 140(2024)

11.
1/2022
Parmentier, G.; Pasquali, A.
Rebounding Cores to Build Star Cluster Multiple Populations
ApJ 924, 81(2022)

10.
11/2020
Parmentier, G.; Pasquali, A.
A New Parameterization of the Star Formation Rate Dense Gas Mass Relation: Embracing Gas Density Gradients
ApJ 903, 56(2020)

9.
4/2020
Parmentier, Geneviève
Molecular Clumps Disguising Their Star Formation Efficiency per Free-fall Time: What We Can Do Not to Be Fooled
ApJ 893, 32(2020)

8.
12/2019
Parmentier, G.
The Density Gradient Inside Molecular-gas Clumps as a Booster of Their Star Formation Activity
ApJ 887, 179(2019)

7.
6/2019
Shukirgaliyev, B.; Parmentier, G.; Berczik, P.; Just, A.
The star cluster survivability after gas expulsion is independent of the impact of the Galactic tidal field
MNRAS 486, 1045(2019)

6.
8/2018
Shukirgaliyev, Bekdaulet; Parmentier, Geneviève et al. (inc. Just, Andreas)
The Long-term Evolution of Star Clusters Formed with a Centrally Peaked Star Formation Efficiency Profile
ApJ 863, 171(2018)

5.
9/2017
Shukirgaliyev, B.; Parmentier, G. et al. (inc. Just, A.)
Impact of a star formation efficiency profile on the evolution of open clusters
A&A 605, A119(2017)

4.
7/2017
Parmentier, G.
The Dense-gas Mass versus Star Formation Rate Relation: A Misleading Linearity?
ApJ 843, 7(2017)

3.
7/2016
Parmentier, G.
A Cautionary Note about Composite Galactic Star Formation Relations
ApJ 826, 74(2016)

2.
8/2014
Parmentier, G.; Pfalzner, S.; Grebel, E. K.
Stellar Age Spreads in Clusters as Imprints of Cluster-parent Clump Densities
ApJ 791, 132(2014)

1.
1/2013
Parmentier, G.; Pfalzner, S.
Local-density-driven clustered star formation
A&A 549, A132(2013)

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