G. Parmentier

1.6k total citations
29 papers, 428 citations indexed

About

G. Parmentier is a scholar working on Astronomy and Astrophysics, Instrumentation and Spectroscopy. According to data from OpenAlex, G. Parmentier has authored 29 papers receiving a total of 428 indexed citations (citations by other indexed papers that have themselves been cited), including 27 papers in Astronomy and Astrophysics, 5 papers in Instrumentation and 2 papers in Spectroscopy. Recurrent topics in G. Parmentier's work include Stellar, planetary, and galactic studies (26 papers), Astrophysics and Star Formation Studies (23 papers) and Galaxies: Formation, Evolution, Phenomena (10 papers). G. Parmentier is often cited by papers focused on Stellar, planetary, and galactic studies (26 papers), Astrophysics and Star Formation Studies (23 papers) and Galaxies: Formation, Evolution, Phenomena (10 papers). G. Parmentier collaborates with scholars based in Germany, Belgium and United Kingdom. G. Parmentier's co-authors include G. Gilmore, Richard de Grijs, Holger Baumgardt, E. K. Grebel, Peter Anders, Susanne Pfalzner, Peter Berczik, Pierre Magain, A. Just and Anne Thoul and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

G. Parmentier

27 papers receiving 413 citations

Peers

G. Parmentier

INSTR

SPECT

NHEP

SNP

Yuri N. Efremov Russia

Gioacchino Accurso United Kingdom

Rosa A. González‐Lópezlira Mexico

L. Morbidelli Italy

Drew Brisbin United States

Piyush Sharda Australia

M. Fumana Italy

N. Miret-Roig Spain

L. Guzmán-Ramírez United Kingdom

Toshiki Saito Japan

Yuri N. Efremov Russia

G. Parmentier

563 ×1.4

160 ×1.1

INSTR

14 ×0.8

SPECT

18 ×1.2

NHEP

13 ×1.9

SNP

Citations per year, relative to G. Parmentier G. Parmentier (= 1×) peers Yuri N. Efremov

Countries citing papers authored by G. Parmentier

Since Specialization

Citations

This map shows the geographic impact of G. Parmentier's research. It shows the number of citations coming from papers published by authors working in each country. You can also color the map by specialization and compare the number of citations received by G. Parmentier with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Parmentier more than expected).

Fields of papers citing papers by G. Parmentier

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Parmentier. Nodes represent research fields, and links connect fields that are likely to share authors. Colored nodes show fields that tend to cite the papers produced by G. Parmentier. The network helps show where G. Parmentier may publish in the future.

Co-authorship network of co-authors of G. Parmentier

This figure shows the co-authorship network connecting the top 25 collaborators of G. Parmentier. A scholar is included among the top collaborators of G. Parmentier based on the total number of citations received by their joint publications. Widths of edges represent the number of papers authors have co-authored together. Node borders signify the number of papers an author published with G. Parmentier. G. Parmentier is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

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20 of 20 papers shown

Parmentier, G.. (2024). Cracking the Relation between Mass and 1P-star Fraction of Globular Clusters. II. The Masses in 1P and 2P Stars as a Second Tool. The Astrophysical Journal. 976(2). 191–191.

Parmentier, G.. (2024). Cracking the Relation between Mass and 1P Star Fraction of Globular Clusters. I. Present-day Cluster Masses as a First Tool. The Astrophysical Journal. 964(2). 140–140. 3 indexed citations

Parmentier, G., et al.. (2019). The star cluster survivability after gas expulsion is independent of the impact of the Galactic tidal field. Monthly Notices of the Royal Astronomical Society. 486(1). 1045–1052. 11 indexed citations

Parmentier, G., et al.. (2017). Impact of a star formation efficiency profile on the evolution of open clusters. Astronomy and Astrophysics. 605. A119–A119. 42 indexed citations

Parmentier, G.. (2017). The Dense-gas Mass versus Star Formation Rate Relation: A Misleading Linearity?. The Astrophysical Journal. 843(1). 7–7. 4 indexed citations

Parmentier, G.. (2014). Local‐density driven clustered star formation: Model and (some) implications. Astronomische Nachrichten. 335(5). 543–548. 4 indexed citations

Parmentier, G. & Susanne Pfalzner. (2012). Local-density-driven clustered star formation. Astronomy and Astrophysics. 549. A132–A132. 38 indexed citations

Parmentier, G. & Holger Baumgardt. (2012). The mass function and dynamical mass of young star clusters: why their initial crossing-time matters crucially. Monthly Notices of the Royal Astronomical Society. 427(3). 1940–1952. 9 indexed citations

Parmentier, G., et al.. (2012). The evolution of the surface brightness of a star cluster as a result of residual star-forming gas expulsion. Monthly Notices of the Royal Astronomical Society. 423(3). 1985–1991. 8 indexed citations

10.

Parmentier, G., et al.. (2008). WHEN EFFICIENT STAR FORMATION DRIVES CLUSTER FORMATION. The Astrophysical Journal. 690(2). 1112–1118. 10 indexed citations

11.

Parmentier, G. & G. Gilmore. (2007). The origin of the Gaussian initial mass function of old globular cluster systems. Monthly Notices of the Royal Astronomical Society. 377(1). 352–372. 35 indexed citations

12.

Jehin, Emmanuël, et al.. (2005). Abundance correlations in mildly metal-poor stars. Astronomy and Astrophysics. 433(1). 285–295. 5 indexed citations

13.

Parmentier, G. & G. Gilmore. (2005). New light on the initial mass function of the Galactic halo globular clusters. Monthly Notices of the Royal Astronomical Society. 363(1). 326–336. 17 indexed citations

14.

Parmentier, G. & E. K. Grebel. (2005). On the origin of the radial mass density profile of the Galactic halo globular cluster system. Monthly Notices of the Royal Astronomical Society. 359(2). 615–623. 8 indexed citations

15.

Parmentier, G.. (2004). Self-enrichment of Galactic halo globular clusters: stimulated star formation and consequences for the halo metallicity distribution. Monthly Notices of the Royal Astronomical Society. 351(2). 585–598. 15 indexed citations

16.

Thoul, Anne, A. Jorissen, S. Goriely, et al.. (2002). Accretion of gas by globular cluster stars. Astronomy and Astrophysics. 383(2). 491–501. 45 indexed citations

17.

Parmentier, G. & G. Gilmore. (2001). The self-enrichment of galactic halo globular clusters. Astronomy and Astrophysics. 378(1). 97–101. 4 indexed citations

18.

Noels, A., et al.. (2000). The Galactic Halo : from Globular Clusters to Field Stars. 35. 30 indexed citations

19.

Parmentier, G., Emmanuël Jehin, Pierre Magain, A. Noels, & Anne Thoul. (2000). Were the Old Halo globular clusters able to sustain a self-enrichment phase?. New Astronomy Reviews. 44(4-6). 351–353. 1 indexed citations

20.

Parmentier, G., et al.. (2000). The Old Halo metallicity gradient: the trace of a self-enrichment process. arXiv (Cornell University). 363. 526.

Rankless uses publication and citation data sourced from OpenAlex, an open and comprehensive bibliographic database. While OpenAlex provides broad and valuable coverage of the global research landscape, it—like all bibliographic datasets—has inherent limitations. These include incomplete records, variations in author disambiguation, differences in journal indexing, and delays in data updates. As a result, some metrics and network relationships displayed in Rankless may not fully capture the entirety of a scholar's output or impact.

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