Xufen Wu

693 total citations
22 papers, 380 citations indexed

About

Xufen Wu is a scholar working on Astronomy and Astrophysics, Instrumentation and Nuclear and High Energy Physics. According to data from OpenAlex, Xufen Wu has authored 22 papers receiving a total of 380 indexed citations (citations by other indexed papers that have themselves been cited), including 21 papers in Astronomy and Astrophysics, 5 papers in Instrumentation and 3 papers in Nuclear and High Energy Physics. Recurrent topics in Xufen Wu's work include Galaxies: Formation, Evolution, Phenomena (18 papers), Stellar, planetary, and galactic studies (10 papers) and Astrophysics and Star Formation Studies (8 papers). Xufen Wu is often cited by papers focused on Galaxies: Formation, Evolution, Phenomena (18 papers), Stellar, planetary, and galactic studies (10 papers) and Astrophysics and Star Formation Studies (8 papers). Xufen Wu collaborates with scholars based in China, Germany and United Kingdom. Xufen Wu's co-authors include Pavel Kroupa, Hongsheng Zhao, Benoît Famaey, Gianfranco Gentile, Hagai B. Perets, Thorsten Naab, Akram Hasani Zonoozi, N. Lyskova, Ludwig Oser and Jörg Dabringhausen and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Journal of Cosmology and Astroparticle Physics.

In The Last Decade

Xufen Wu

18 papers receiving 354 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Xufen Wu China 11 367 119 94 21 6 22 380
Nina Roth United Kingdom 7 316 0.9× 155 1.3× 42 0.4× 29 1.4× 3 0.5× 9 324
Alex Krolewski Canada 9 211 0.6× 43 0.4× 91 1.0× 16 0.8× 7 1.2× 21 223
Akram Hasani Zonoozi Iran 14 553 1.5× 214 1.8× 75 0.8× 19 0.9× 6 1.0× 37 575
Daniele Sorini United Kingdom 10 268 0.7× 77 0.6× 96 1.0× 17 0.8× 6 1.0× 17 285
Salvador Salazar-Albornoz Germany 6 220 0.6× 86 0.7× 68 0.7× 14 0.7× 3 0.5× 6 229
Alexander Arth Germany 4 288 0.8× 126 1.1× 60 0.6× 23 1.1× 3 0.5× 5 305
Kazuyuki Akitsu Japan 11 257 0.7× 65 0.5× 101 1.1× 13 0.6× 10 1.7× 18 277
Rossana Ruggeri Australia 8 225 0.6× 71 0.6× 75 0.8× 22 1.0× 4 0.7× 14 244
K. Migkas Germany 8 280 0.8× 56 0.5× 147 1.6× 16 0.8× 18 3.0× 13 288
Saroj Adhikari United States 6 234 0.6× 62 0.5× 81 0.9× 12 0.6× 6 1.0× 8 241

Countries citing papers authored by Xufen Wu

Since Specialization
Citations

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

Fields of papers citing papers by Xufen Wu

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Xufen Wu

This figure shows the co-authorship network connecting the top 25 collaborators of Xufen Wu. A scholar is included among the top collaborators of Xufen Wu 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 Xufen Wu. Xufen Wu 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.
2.
Wu, Xufen, et al.. (2024). Formation of collisional ring galaxies in Milgromian dynamics. Monthly Notices of the Royal Astronomical Society. 528(1). 620–633. 1 indexed citations
3.
Wu, Xufen, et al.. (2024). Energy Evolution in the Progenitor of Galaxy Shells: A Semi-analytical Model. The Astrophysical Journal. 975(1). 11–11. 1 indexed citations
4.
5.
Wu, Xufen, et al.. (2022). Collisions of Young Disk Galaxies in the Early Universe. The Astrophysical Journal. 926(2). 224–224. 1 indexed citations
6.
Kroupa, Pavel, Tereza Jeřabková, Ingo Thies, et al.. (2022). Asymmetrical tidal tails of open star clusters: stars crossing their cluster’s práh† challenge Newtonian gravitation. Monthly Notices of the Royal Astronomical Society. 517(3). 3613–3639. 36 indexed citations
7.
Haghi, Hosein, Pavel Kroupa, Indranil Banik, et al.. (2019). A new formulation of the external field effect in MOND and numerical simulations of ultra-diffuse dwarf galaxies – application to NGC 1052-DF2 and NGC 1052-DF4. Monthly Notices of the Royal Astronomical Society. 487(2). 2441–2454. 34 indexed citations
8.
Wu, Xufen & Pavel Kroupa. (2019). The kinematics of star clusters undergoing gas expulsion in Newtonian and Milgromian dynamics. Monthly Notices of the Royal Astronomical Society. 487(3). 4012–4024. 2 indexed citations
9.
Kroupa, Pavel, Indranil Banik, Hosein Haghi, et al.. (2018). A common Milgromian acceleration scale in nature. Nature Astronomy. 2(12). 925–926. 25 indexed citations
10.
Liu, Wenjuan, Hongyan Zhou, Ning Jiang, et al.. (2016). SDSS J163459.82+204936.0: A RINGED INFRARED-LUMINOUS QUASAR WITH OUTFLOWS IN BOTH ABSORPTION AND EMISSION LINES. The Astrophysical Journal. 822(2). 64–64. 6 indexed citations
11.
Wu, Xufen, Ortwin Gerhard, Thorsten Naab, et al.. (2014). The mass and angular momentum distribution of simulated massive early-type galaxies to large radii. Monthly Notices of the Royal Astronomical Society. 438(3). 2701–2715. 53 indexed citations
12.
Wu, Xufen & Pavel Kroupa. (2014). Galactic rotation curves, the baryon-to-dark-halo-mass relation and space–time scale invariance. Monthly Notices of the Royal Astronomical Society. 446(1). 330–344. 44 indexed citations
13.
Wu, Xufen & Pavel Kroupa. (2013). The specific frequency and the globular cluster formation efficiency in Milgromian dynamics. Monthly Notices of the Royal Astronomical Society. 435(2). 1536–1540. 7 indexed citations
14.
Wu, Xufen & Pavel Kroupa. (2013). The dynamical phase transitions of stellar systems and the corresponding kinematics. Monthly Notices of the Royal Astronomical Society. 435(1). 728–742. 15 indexed citations
15.
Zhao, Hongsheng, et al.. (2012). StirringN-body systems: universality of end states. Monthly Notices of the Royal Astronomical Society. 424(3). 1737–1751. 3 indexed citations
16.
Wu, Xufen, Hongsheng Zhao, & Benoît Famaey. (2010). Lopsidedness of cluster galaxies in modified gravity. Journal of Cosmology and Astroparticle Physics. 2010(6). 10–10. 14 indexed citations
17.
Bienaymé, O., Benoît Famaey, Xufen Wu, Hongsheng Zhao, & Dominique Aubert. (2009). Galactic kinematics with modified Newtonian dynamics. Springer Link (Chiba Institute of Technology). 19 indexed citations
18.
Wu, Xufen, Hongsheng Zhao, Yougang Wang, Claudio Llinares, & Alexander Knebe. (2009). N-body simulations for testing the stability of triaxial galaxies in MOND. Monthly Notices of the Royal Astronomical Society. 396(1). 109–120. 10 indexed citations
19.
Wu, Xufen, Benoît Famaey, Gianfranco Gentile, Hagai B. Perets, & Hongsheng Zhao. (2008). Milky Way potentials in cold dark matter and MOdified Newtonian Dynamics. Is the Large Magellanic Cloud on a bound orbit?. Monthly Notices of the Royal Astronomical Society. 386(4). 2199–2208. 65 indexed citations
20.
Wu, Xufen, Hongsheng Zhao, Benoît Famaey, et al.. (2007). Loss of Mass and Stability of Galaxies in Modified Newtonian Dynamics. The Astrophysical Journal. 665(2). L101–L104. 34 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.

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