Ding-Xiong Wang

582 total citations
62 papers, 385 citations indexed

About

Ding-Xiong Wang is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Geophysics. According to data from OpenAlex, Ding-Xiong Wang has authored 62 papers receiving a total of 385 indexed citations (citations by other indexed papers that have themselves been cited), including 60 papers in Astronomy and Astrophysics, 35 papers in Nuclear and High Energy Physics and 5 papers in Geophysics. Recurrent topics in Ding-Xiong Wang's work include Astrophysical Phenomena and Observations (55 papers), Pulsars and Gravitational Waves Research (46 papers) and Astrophysics and Cosmic Phenomena (28 papers). Ding-Xiong Wang is often cited by papers focused on Astrophysical Phenomena and Observations (55 papers), Pulsars and Gravitational Waves Research (46 papers) and Astrophysics and Cosmic Phenomena (28 papers). Ding-Xiong Wang collaborates with scholars based in China, United States and India. Ding-Xiong Wang's co-authors include Wei‐Hua Lei, Qingwen Wu, Yuan-Chuan Zou, Xinwu Cao, Bing Zhang, Wei Xie, Luis C. Ho, En‐Wei Liang, Hou-Jun Lü and He Gao and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Letters.

In The Last Decade

Ding-Xiong Wang

53 papers receiving 366 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
Ding-Xiong Wang China 11 372 203 19 16 11 62 385
Alejandra Jiménez-Rosales Germany 8 289 0.8× 170 0.8× 19 1.0× 19 1.2× 8 0.7× 11 300
Vojtěch Witzany Czechia 10 290 0.8× 114 0.6× 15 0.8× 13 0.8× 25 2.3× 17 310
Gibwa Musoke Netherlands 8 338 0.9× 184 0.9× 22 1.2× 25 1.6× 5 0.5× 12 357
J. W. Broderick Australia 13 475 1.3× 266 1.3× 25 1.3× 34 2.1× 3 0.3× 39 494
P. M. Plewa Germany 7 296 0.8× 137 0.7× 8 0.4× 18 1.1× 9 0.8× 12 306
O. Straub Czechia 14 525 1.4× 286 1.4× 33 1.7× 43 2.7× 9 0.8× 23 534
Masaaki Sakano Japan 9 438 1.2× 180 0.9× 33 1.7× 17 1.1× 2 0.2× 18 446
D. Kunneriath Czechia 12 410 1.1× 156 0.8× 42 2.2× 40 2.5× 6 0.5× 28 416
Steven V. Fuerst United Kingdom 6 342 0.9× 181 0.9× 6 0.3× 20 1.3× 3 0.3× 6 352
J. Kolodziejczak United States 5 172 0.5× 67 0.3× 16 0.8× 14 0.9× 6 0.5× 10 209

Countries citing papers authored by Ding-Xiong Wang

Since Specialization
Citations

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

Fields of papers citing papers by Ding-Xiong Wang

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by Ding-Xiong Wang. 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 Ding-Xiong Wang. The network helps show where Ding-Xiong Wang may publish in the future.

Co-authorship network of co-authors of Ding-Xiong Wang

This figure shows the co-authorship network connecting the top 25 collaborators of Ding-Xiong Wang. A scholar is included among the top collaborators of Ding-Xiong Wang 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 Ding-Xiong Wang. Ding-Xiong Wang 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.
Xie, Wei, Wei‐Hua Lei, & Ding-Xiong Wang. (2017). What Can We Learn about GRB from the Variability Timescale Related Correlations?. The Astrophysical Journal. 838(2). 143–143. 7 indexed citations
2.
Xie, Wei, Wei‐Hua Lei, & Ding-Xiong Wang. (2016). NUMERICAL AND ANALYTICAL SOLUTIONS OF NEUTRINO-DOMINATED ACCRETION FLOWS WITH A NON-ZERO TORQUE BOUNDARY CONDITION AND ITS APPLICATIONS IN GAMMA-RAY BURSTS. The Astrophysical Journal. 833(2). 129–129. 11 indexed citations
3.
Wu, Qingwen, et al.. (2014). Modelling the ‘outliers’ track of the radio–X-ray correlation in X-ray binaries based on a disc–corona model. Monthly Notices of the Royal Astronomical Society. 440(2). 965–970. 14 indexed citations
4.
Lei, Wei‐Hua, et al.. (2014). QUASI-PERIODIC VARIATIONS IN X-RAY EMISSION AND LONG-TERM RADIO OBSERVATIONS: EVIDENCE FOR A TWO-COMPONENT JET IN Sw J1644+57. The Astrophysical Journal. 788(1). 32–32. 26 indexed citations
5.
Xie, Wei, et al.. (2012). A two-component jet model based on the Blandford-Znajek and Blandford-Payne processes. Research in Astronomy and Astrophysics. 12(7). 817–828. 12 indexed citations
6.
Li, Yang, Zhaoming Gan, & Ding-Xiong Wang. (2009). A simplified model of ADAF with the jet driven by the large-scale magnetic field. New Astronomy. 15(1). 102–107.
7.
Wang, Ding-Xiong, et al.. (2008). The BZ–MC–BP model for jet production from a black hole accretion disc. Monthly Notices of the Royal Astronomical Society. 385(2). 841–848. 5 indexed citations
8.
Wang, Ding-Xiong, et al.. (2008). A Toy Model for Magnetic Field Configurations in Black Hole Accretion Discs. Chinese Physics Letters. 25(6). 2327–2330. 1 indexed citations
9.
Ye, Yongchun, et al.. (2005). Magnetic extraction of energy from black hole accretion disc and its application to astrophysics. Chinese Physics. 14(2). 439–447. 2 indexed citations
10.
Wang, Ding-Xiong, et al.. (2005). A model of rotating hotspots for the 3 : 2 frequency ratio of high-frequency quasi-periodic oscillations in black hole X-ray binaries. Monthly Notices of the Royal Astronomical Society. 359(1). 36–42. 3 indexed citations
11.
Wang, Ding-Xiong, et al.. (2004). Magnetic Extraction of Energy from Accretion Disc Around a Rotating Black Hole. Chinese Physics Letters. 21(9). 1861–1864. 2 indexed citations
12.
Wang, Ding-Xiong, et al.. (2004). A toy model for magnetic extraction of energy from black hole accretion disk. New Astronomy. 9(8). 585–597. 4 indexed citations
13.
Wang, Ding-Xiong, et al.. (2003). An analytic model of a rotating hotspot and kilohertz quasi-periodic oscillations in X-ray binaries. Monthly Notices of the Royal Astronomical Society. 344(2). 473–480. 10 indexed citations
14.
Wang, Ding-Xiong, et al.. (2002). Two Mechanisms for Extracting Energy and Angular Momentum from a Rotating Black Hole. General Relativity and Gravitation. 34(5). 619–632.
15.
Wang, Ding-Xiong, et al.. (2000). A study on the oscillatory instability of a hot two-temperature accretion disk including advection. Chinese Astronomy and Astrophysics. 24(1). 23–29. 1 indexed citations
16.
Wang, Ding-Xiong. (2000). Relations between Black Hole Spin and Angular Velocity of Accreting Particles near the Horizon. General Relativity and Gravitation. 32(4). 553–563. 1 indexed citations
17.
Wang, Ding-Xiong, et al.. (1999). Entropy Change of Black Holes in Disk-Accretion. Chinese Physics Letters. 16(6). 464–466. 1 indexed citations
18.
Wang, Ding-Xiong. (1998). Evolution of Dimensionless Angular Momentum of Central Black Holes of Accretion Disks. General Relativity and Gravitation. 30(7). 1025–1035. 7 indexed citations
19.
Wang, Ding-Xiong. (1992). Self-Gravitating Electromagnetic Radiation Systems of Spherical Symmetry Before Gravitational Collapse to Black-Holes. 12(3). 202–206.
20.
Sabbata, V. de, Ding-Xiong Wang, & C. Sivaram. (1990). Torsion Effects in Black Hole Evaporation. Annalen der Physik. 502(6). 508–510. 2 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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