G. Vauclair

3.5k total citations
79 papers, 921 citations indexed

About

G. Vauclair is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, G. Vauclair has authored 79 papers receiving a total of 921 indexed citations (citations by other indexed papers that have themselves been cited), including 70 papers in Astronomy and Astrophysics, 41 papers in Instrumentation and 8 papers in Computational Mechanics. Recurrent topics in G. Vauclair's work include Stellar, planetary, and galactic studies (68 papers), Astronomy and Astrophysical Research (41 papers) and Astrophysics and Star Formation Studies (26 papers). G. Vauclair is often cited by papers focused on Stellar, planetary, and galactic studies (68 papers), Astronomy and Astrophysical Research (41 papers) and Astrophysics and Star Formation Studies (26 papers). G. Vauclair collaborates with scholars based in France, United States and Canada. G. Vauclair's co-authors include S. Vauclair, G. Michaud, S. Charpinet, Weikai Zong, Y. Charland, V. Van Grootel, N. Dolez, N. Giammichele, F. C. Wachlin and G. Fontaine and has published in prestigious journals such as SHILAP Revista de lepidopterología, The Astrophysical Journal and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

G. Vauclair

71 papers receiving 872 citations

Author Peers

Peers are selected by citation overlap in the author's most active subfields. citations · hero ref

Author Last Decade Papers Cites
G. Vauclair 902 378 51 49 48 79 921
R. Raddi 1.4k 1.6× 556 1.5× 67 1.3× 43 0.9× 51 1.1× 61 1.5k
Jiřı́ Krtička 1.4k 1.6× 393 1.0× 82 1.6× 35 0.7× 56 1.2× 110 1.5k
F. van Wyk 1.1k 1.2× 443 1.2× 104 2.0× 26 0.5× 37 0.8× 71 1.1k
A. M. Cool 1.0k 1.1× 344 0.9× 30 0.6× 72 1.5× 90 1.9× 39 1.1k
H. F. Henrichs 1.3k 1.4× 304 0.8× 115 2.3× 49 1.0× 30 0.6× 59 1.3k
Elena Cukanovaite 791 0.9× 358 0.9× 50 1.0× 28 0.6× 42 0.9× 15 839
V. V. Tsymbal 947 1.0× 346 0.9× 46 0.9× 28 0.6× 23 0.5× 49 979
Leigh C. Smith 950 1.1× 407 1.1× 64 1.3× 13 0.3× 34 0.7× 65 982
K. M. Cudworth 1.2k 1.3× 571 1.5× 43 0.8× 10 0.2× 65 1.4× 48 1.2k
G. Roberts 781 0.9× 200 0.5× 76 1.5× 18 0.4× 114 2.4× 39 800

Countries citing papers authored by G. Vauclair

Since Specialization
Citations

This map shows the geographic impact of G. Vauclair'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. Vauclair with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites G. Vauclair more than expected).

Fields of papers citing papers by G. Vauclair

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by G. Vauclair. 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. Vauclair. The network helps show where G. Vauclair may publish in the future.

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

This figure shows the co-authorship network connecting the top 25 collaborators of G. Vauclair. A scholar is included among the top collaborators of G. Vauclair 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. Vauclair. G. Vauclair is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

20 of 20 papers shown
1.
Wachlin, F. C., G. Vauclair, S. Vauclair, & L. G. Althaus. (2022). New simulations of accreting DA white dwarfs: Inferring accretion rates from the surface contamination. Astronomy and Astrophysics. 660. A30–A30. 6 indexed citations
2.
Wachlin, F. C., G. Vauclair, S. Vauclair, & L. G. Althaus. (2017). Importance of fingering convection for accreting white dwarfs in the framework of full evolutionary calculations: the case of the hydrogen-rich white dwarfs GD 133 and G 29-38. Springer Link (Chiba Institute of Technology). 19 indexed citations
3.
Deal, Morgan, et al.. (2017). Asteroseismology of the exoplanet-host F-type star 94 Ceti: Impact of atomic diffusion on the stellar parameters. Astronomy and Astrophysics. 601. A127–A127. 9 indexed citations
4.
Zong, Weikai, S. Charpinet, & G. Vauclair. (2016). Signatures of nonlinear mode interactions in the pulsating hot B subdwarf star KIC 10139564. Springer Link (Chiba Institute of Technology). 32 indexed citations
5.
Giammichele, N., G. Fontaine, P. Bergeron, et al.. (2015). A NEW ANALYSIS OF THE TWO CLASSICAL ZZ CETI WHITE DWARFS GD 165 AND ROSS 548. I. PHOTOMETRY AND SPECTROSCOPY. The Astrophysical Journal. 815(1). 56–56. 9 indexed citations
6.
Deal, Morgan, S. Deheuvels, G. Vauclair, S. Vauclair, & F. C. Wachlin. (2013). Accretion from debris disks onto white dwarfs. Astronomy and Astrophysics. 557. L12–L12. 37 indexed citations
7.
Vauclair, G., J. E. Solheim, N. Dolez, et al.. (2012). Period and Amplitude Changes in the GW Vir Variable Star PG 0122+200: Evidence for Resonant Coupling. ASPC. 462. 160. 1 indexed citations
8.
Théado, S., S. Vauclair, J. Ballot, et al.. (2012). Precise modeling of the exoplanet host star and CoRoT main target HD 52265. Astronomy and Astrophysics. 543. A96–A96. 20 indexed citations
9.
Charpinet, S., A Baglin, V. Van Grootel, et al.. (2010). CoRoT opens a new era in hot B subdwarf asteroseismology. Astronomy and Astrophysics. 516. L6–L6. 37 indexed citations
10.
Dolez, N., S. Vauclair, E. Michel, et al.. (2009). HD 51106 and HD 50747: an ellipsoidal binary and a triple system observed with CoRoT. Astronomy and Astrophysics. 506(1). 159–165. 2 indexed citations
11.
Vauclair, S., F. Bouchy, G. Vauclair, et al.. (2008). The exoplanet-host starιHorologii: an evaporated member of the primordial Hyades cluster. Astronomy and Astrophysics. 482(2). L5–L8. 35 indexed citations
12.
Vauclair, S., et al.. (2007). The CoRoT primary target HD 52265: models and seismic tests. Springer Link (Chiba Institute of Technology). 13 indexed citations
13.
Solheim, J.‐E., et al.. (2007). Abell 43: longest period planetary nebula nucleus variable. Springer Link (Chiba Institute of Technology). 3 indexed citations
14.
Córsico, A. H., M. M. Miller Bertolami, L. G. Althaus, G. Vauclair, & K. Werner. (2007). Asteroseismological constraints on the coolest GW Virginis variable star (PG 1159-type) PG 0122+200. Astronomy and Astrophysics. 475(2). 619–627. 22 indexed citations
15.
Vauclair, G., et al.. (2006). The ZZ Ceti star G 185-32: new insight from asteroseismology. Astronomy and Astrophysics. 453(1). 219–227. 10 indexed citations
16.
Vauclair, G., et al.. (2006). Asteroseismological constraints on the structure of the ZZ Ceti star HL Tau 76. Astronomy and Astrophysics. 446(1). 223–235. 13 indexed citations
17.
Vauclair, G., J.‐E. Solheim, & R. H. Østensen. (2005). Abell 43, a second pulsating “hybrid-PG 1159” star. Astronomy and Astrophysics. 433(3). 1097–1100. 12 indexed citations
18.
Vauclair, G., N. Dolez, Jian-Ning Fu, et al.. (2000). PG 1541+650: A new ZZ Ceti white dwarf. SHILAP Revista de lepidopterología. 1 indexed citations
19.
Dolez, N., et al.. (1998). Asteroseismology of DAV White Dwarfs with Time-Frequency Analysis and Band-Limited Interpolation. ASPC. 135. 442.
20.
Holberg, J. B., E. M. Sion, James Liebert, & G. Vauclair. (1987). EXOSAT Observations of DA White Dwarf Stars and the m(He)/n(H)vs. Teff Correlation. Bulletin of the American Astronomical Society. 19. 1041.

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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