Priv.-Doz. Dr. Eng. Geneviève Parmentier
ORCID: 0000-0002-2152-4298
"Do not follow where the path may lead.
Go, instead, where there is no path and leave a trail."
Ralph Waldo Emerson (1803 - 1882)
Thank you to Stefan Jordan for having taken the picture
Recent News
Cracking the relation between mass and 1P-star fraction of globular clusters:
II. The masses in 1P and 2P stars as a second tool,
accepted for publication in The Astrophysical Journal, arxiv:2410.11950
Cracking the relation between mass and 1P-star fraction of globular clusters:
I. Present-day cluster masses as a first tool,
accepted for publication in The Astrophysical Journal, arxiv:2402.07979
Lund Observatory Källén Seminars for Young Astronomers (slides, September 2022)
"Rebounding Cores to Build Star Cluster Multiple Populations"
"Rebounding Cores to Build Star Cluster Multiple Populations",
by Parmentier and Pasquali, accepted for publication in The Astrophysical Journal, arxiv:2110.14470
Chalmers Astrophysics Colloquium (slides, October 2020; also Lund Observatory: March 2021 and March 2022)
"The Density Gradient Inside Molecular-Gas Clumps as a Booster of their Star Formation Activity"
"A new parameterization of the star formation rate-dense gas mass relation: embracing gas density gradients",
by Parmentier and Pasquali, accepted for publication in The Astrophysical Journal, arxiv:2009.10652
Astronomisches Rechen-Institut Kolloquium (slides, July 2020)
"The Density Gradient Inside Molecular-Gas Clumps as a Booster of their Star Formation Activity"
"Molecular clumps disguising their star formation efficiency per freefall time: What we can do not to be fooled",
accepted for publication in The Astrophysical Journal, arxiv:2003.01613
"The density gradient inside molecular-gas clumps as a booster of their star formation activity",
accepted for publication in The Astrophysical Journal: arxiv:1911.04994
ESO Observing-Programmes-Committee panel member (somewhere in the past)
"The star cluster survivability after gas expulsion is independent of the impact of the Galactic tidal field",
3rd paper of my PhD student: Shukirgalieyv, Parmentier, Berczik & Just,
accepted for publication in The Astrophysical Journal: arXiv:1903.09560
Contributed Talk "Cluster Formation with a Constant Star Formation Efficiency per Free-Fall Time",
at Star Cluster Formation: Mapping the first few Myrs (Grenoble, August 2018) and
Contributed Talk "4 Star Formation Relations (+ Strengthened Cluster Survival) With One Single Model"
at The Wonders of Star Formation, Edinburgh, September 2018 (slides: both talks merged in one single presentation)
"The long-term evolution of star clusters formed with a centrally-peaked star-formation-efficiency profile",
2nd paper of my PhD student: Shukirgalieyv, Parmentier, Just & Berczik,
accepted for publication in The Astrophysical Journal: arXiv:1807.04755
Invited Lecturer
at 11th HGSFP Winterschool,
Obergurgl, Austria, January 26-30, 2018
Invited Talk "The Early Survival of (Globular) Star Clusters: Easier Than We Thought!",
at Globular cluster systems and their host galaxies, Sexten, June 2017 (slides)
"The impact of a star-formation efficiency profile on the evolution of open clusters",
1st paper of my PhD student: Shukirgalieyv, Parmentier, Just & Berczik,
accepted for publication in Astronomy & Astrophysics: arXiv:1706.03228
"The dense-gas mass versus star formation rate relation: a misleading linearity?",
accepted for publication in The Astrophysical Journal: arXiv:1705.10827
Invited Lecturer at 10th HGSFP Winterschool,
Obergurgl, Austria, January 27-31, 2017
"A cautionary note about composite Galactic star formation relations",
accepted for publication in The Astrophysical Journal: arXiv:1605.07623
Contact Details
Address: | Mönchhofstrasse 12-14 |
| D-69120 Heidelberg - Germany |
Tel: | (+49 6221) 54 - 1836 |
Fax: | (+49 6221) 54 - 1888 |
E-mail: | gparm _(AT)_ ari.uni-heidelberg.de |
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ORCID: | 0000-0002-2152-4298 |