F. C. Wachlin

553 total citations
21 papers, 395 citations indexed

About

F. C. Wachlin is a scholar working on Astronomy and Astrophysics, Statistical and Nonlinear Physics and Instrumentation. According to data from OpenAlex, F. C. Wachlin has authored 21 papers receiving a total of 395 indexed citations (citations by other indexed papers that have themselves been cited), including 16 papers in Astronomy and Astrophysics, 6 papers in Statistical and Nonlinear Physics and 4 papers in Instrumentation. Recurrent topics in F. C. Wachlin's work include Stellar, planetary, and galactic studies (14 papers), Astrophysics and Star Formation Studies (9 papers) and Astro and Planetary Science (8 papers). F. C. Wachlin is often cited by papers focused on Stellar, planetary, and galactic studies (14 papers), Astrophysics and Star Formation Studies (9 papers) and Astro and Planetary Science (8 papers). F. C. Wachlin collaborates with scholars based in Argentina, France and Spain. F. C. Wachlin's co-authors include L. G. Althaus, M. M. Miller Bertolami, A. H. Córsico, María E. Camisassa, P. M. Cincotta, S. Vauclair, R. D. Rohrmann, E. Garcı́a–Berro, G. Vauclair and S. Ferraz‐Mello 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

F. C. Wachlin

21 papers receiving 369 citations

Peers — A (Enhanced Table)

Peers by citation overlap · career bar shows stage (early→late) cites · hero ref

Name	h						Papers	Cites
F. C. Wachlin Argentina	10	316	88	48	16	15	21	395
R. de Souza Brazil	12	319 1.0×	134 1.5×	36 0.8×	21 1.3×	7 0.5×	42	355
James Annis United States	8	349 1.1×	152 1.7×	11 0.2×	68 4.3×	10 0.7×	9	468
M. Moshir United States	10	316 1.0×	73 0.8×	39 0.8×	59 3.7×	4 0.3×	19	394
I. Berentzen Germany	9	341 1.1×	149 1.7×	25 0.5×	22 1.4×	8 0.5×	16	373
L. Faccioli France	9	175 0.6×	88 1.0×	9 0.2×	33 2.1×	12 0.8×	22	229
Maxime Rischard United States	5	125 0.4×	57 0.6×	7 0.1×	14 0.9×	5 0.3×	5	207
Hideki Yahagi Japan	9	162 0.5×	72 0.8×	17 0.4×	25 1.6×	13 0.9×	14	193
S. W. Hodson United States	11	235 0.7×	85 1.0×	10 0.2×	35 2.2×	4 0.3×	35	409
I. Sevilla-Noarbe Spain	9	169 0.5×	56 0.6×	13 0.3×	17 1.1×	20 1.3×	27	215
Bruno Régaldo-Saint Blancard United States	10	175 0.6×	39 0.4×	42 0.9×	38 2.4×	8 0.5×	14	237

Countries citing papers authored by F. C. Wachlin

Since Specialization

Citations

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

Fields of papers citing papers by F. C. Wachlin

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by F. C. Wachlin. 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 F. C. Wachlin. The network helps show where F. C. Wachlin may publish in the future.

Co-authorship network of co-authors of F. C. Wachlin

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

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

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

Bertolami, M. M. Miller, et al.. (2022). An evolutionary channel for CO-rich and pulsating He-rich subdwarfs. Monthly Notices of the Royal Astronomical Society Letters. 511(1). L60–L65. 14 indexed citations

Camisassa, María E., L. G. Althaus, A. H. Córsico, et al.. (2019). The evolution of ultra-massive white dwarfs. Springer Link (Chiba Institute of Technology). 89 indexed citations

Córsico, A. H., et al.. (2018). Pulsation properties of ultra-massive DA white dwarf stars with ONe cores. Astronomy and Astrophysics. 621. A100–A100. 21 indexed citations

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

Camisassa, María E., L. G. Althaus, R. D. Rohrmann, et al.. (2017). Updated Evolutionary Sequences for Hydrogen-deficient White Dwarfs. The Astrophysical Journal. 839(1). 11–11. 39 indexed citations

Wachlin, F. C., S. Vauclair, & L. G. Althaus. (2014). Fingering convection in red giants revisited. Astronomy and Astrophysics. 570. A58–A58. 15 indexed citations

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

Wachlin, F. C., M. M. Miller Bertolami, & L. G. Althaus. (2011). Thermohaline mixing and the photospheric composition of low-mass giant stars. Astronomy and Astrophysics. 533. A139–A139. 35 indexed citations

10.

Wachlin, F. C. & D. D. Carpintero. (2006). Softened potentials and the multipolar expansion. LA Referencia (Red Federada de Repositorios Institucionales de Publicaciones Científicas). 42(2). 251–259. 1 indexed citations

11.

Carpintero, D. D. & F. C. Wachlin. (2006). Sensitivity of the orbital content of a model stellar system to the potential approximation used to describe it. Celestial Mechanics and Dynamical Astronomy. 96(2). 129–136. 6 indexed citations

12.

Muzzio, J. C., F. C. Wachlin, & D. D. Carpintero. (2002). DYNAMICS OF GALACTIC SATELLITES ON ELONGATED ORBITS. Redalyc (Universidad Autónoma del Estado de México). 14. 69–69. 1 indexed citations

13.

Muzzio, J. C., et al.. (2001). Stellar Motions in Galactic Satellites. Celestial Mechanics and Dynamical Astronomy. 81(1-2). 167–176. 3 indexed citations

14.

Muzzio, J. C., F. C. Wachlin, & D. D. Carpintero. (2000). Regular and Chaotic Motion in a Restricted Three–Body Problem of Astrophysical Interest. International Astronomical Union Colloquium. 174. 281–285. 5 indexed citations

15.

Carpintero, D. D., J. C. Muzzio, & F. C. Wachlin. (1999). Regular and Chaotic Motion in Globular Clusters. International Astronomical Union Colloquium. 172. 159–168. 1 indexed citations

16.

Carpintero, D. D., J. C. Muzzio, & F. C. Wachlin. (1999). Regular and Chaotic Motion in Globular Clusters. Celestial Mechanics and Dynamical Astronomy. 73(1-4). 159–168. 9 indexed citations

17.

Wachlin, F. C. & S. Ferraz‐Mello. (1998). Frequency map analysis of the orbital structure in elliptical galaxies. Monthly Notices of the Royal Astronomical Society. 298(1). 22–32. 21 indexed citations

18.

Wachlin, F. C. & J. C. Muzzio. (1997). Testing Galactic Oscillations. Celestial Mechanics and Dynamical Astronomy. 67(3). 225–235. 3 indexed citations

19.

Cincotta, P. M., et al.. (1996). Information entropy. Celestial Mechanics and Dynamical Astronomy. 64(1-2). 43–53. 61 indexed citations

20.

Wachlin, F. C., et al.. (1993). A perturbation particle method for stability studies of stellar systems. Monthly Notices of the Royal Astronomical Society. 262(4). 1007–1012. 4 indexed citations

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.

Explore authors with similar magnitude of impact