W. Kley

7.2k total citations · 1 hit paper
134 papers, 4.3k citations indexed

About

W. Kley is a scholar working on Astronomy and Astrophysics, Spectroscopy and Instrumentation. According to data from OpenAlex, W. Kley has authored 134 papers receiving a total of 4.3k indexed citations (citations by other indexed papers that have themselves been cited), including 126 papers in Astronomy and Astrophysics, 11 papers in Spectroscopy and 6 papers in Instrumentation. Recurrent topics in W. Kley's work include Astrophysics and Star Formation Studies (115 papers), Astro and Planetary Science (85 papers) and Stellar, planetary, and galactic studies (81 papers). W. Kley is often cited by papers focused on Astrophysics and Star Formation Studies (115 papers), Astro and Planetary Science (85 papers) and Stellar, planetary, and galactic studies (81 papers). W. Kley collaborates with scholars based in Germany, United Kingdom and United States. W. Kley's co-authors include Richard P. Nelson, Thomas Henning, Hubert Klahr, Gennaro D’Angelo, Gerben Dirksen, D. N. C. Lin, R. Kuiper, B. Bitsch, A. Crida and R. Speith and has published in prestigious journals such as The Astrophysical Journal, Journal of Computational Physics and Monthly Notices of the Royal Astronomical Society.

In The Last Decade

W. Kley

128 papers receiving 4.1k citations

Hit Papers

align trajectories sort by overperformance

What are hit papers?

Hit papers significantly outperform the citation benchmark for their cohort. A paper qualifies if it has ≥500 total citations, achieves ≥1.5× the top-1% citation threshold for papers in the same subfield and year (this is the minimum needed to enter the top 1%, not the average within it), or reaches the top citation threshold in at least one of its specific research topics.

Planet-Disk Interaction and Orbital Evolution

2012 405 citations W. Kley, Richard P. Nelson profile →

Author Peers

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

Author						Papers	Cites
W. Kley	4.2k	505	140	135	123	134	4.3k
Andrew N. Youdin	3.4k 0.8×	388 0.8×	67 0.5×	160 1.2×	137 1.1×	43	3.6k
S. Fromang	2.6k 0.6×	376 0.7×	68 0.5×	78 0.6×	148 1.2×	60	2.8k
Zhaohuan Zhu	3.5k 0.8×	943 1.9×	154 1.1×	64 0.5×	55 0.4×	125	3.6k
A. Meredith Hughes	3.3k 0.8×	942 1.9×	118 0.8×	58 0.4×	33 0.3×	75	3.4k
B. Stelzer	3.2k 0.8×	481 1.0×	296 2.1×	43 0.3×	75 0.6×	115	3.3k
Eugene Chiang	5.4k 1.3×	903 1.8×	333 2.4×	126 0.9×	44 0.4×	92	5.5k
R. Kuiper	2.2k 0.5×	310 0.6×	152 1.1×	38 0.3×	50 0.4×	91	2.3k
C. Pinte	4.1k 1.0×	1.3k 2.6×	180 1.3×	33 0.2×	67 0.5×	146	4.2k
Giovanni Rosotti	2.9k 0.7×	970 1.9×	102 0.7×	27 0.2×	34 0.3×	127	3.0k
P. Ábrahám	1.9k 0.5×	362 0.7×	149 1.1×	53 0.4×	29 0.2×	134	2.0k

Countries citing papers authored by W. Kley

Since Specialization

Citations

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

Fields of papers citing papers by W. Kley

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of W. Kley

This figure shows the co-authorship network connecting the top 25 collaborators of W. Kley. A scholar is included among the top collaborators of W. Kley 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 W. Kley. W. Kley 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

Kuiper, R., et al.. (2021). Steady state by recycling prevents premature collapse of protoplanetary atmospheres. Springer Link (Chiba Institute of Technology). 4 indexed citations

Picogna, Giovanni, et al.. (2021). Giant planet migration during the disc dispersal phase. Springer Link (Chiba Institute of Technology). 1 indexed citations

Lega, Elena, Richard P. Nelson, Alessandro Morbidelli, et al.. (2021). Migration of Jupiter-mass planets in low-viscosity discs. Springer Link (Chiba Institute of Technology). 22 indexed citations

Dullemond, C. P., et al.. (2021). Modeling the nonaxisymmetric structure in the HD 163296 disk with planet-disk interaction. Springer Link (Chiba Institute of Technology). 15 indexed citations

Kley, W. & Nader Haghighipour. (2015). Evolution of circumbinary planets around eccentric binaries: The case of Kepler-34. Springer Link (Chiba Institute of Technology). 30 indexed citations

Сулейманов, В. Ф., et al.. (2014). Modeling the EUV spectra of optically thick boundary layers of dwarf novae in outburst. Springer Link (Chiba Institute of Technology). 13 indexed citations

Daemgen, S., M. G. Petr-Gotzens, S. Correia, et al.. (2013). Protoplanetary disk evolution and stellar parameters of T Tauri binaries in Chamaeleon I. Springer Link (Chiba Institute of Technology). 21 indexed citations

Müller, Tobias W. A. & W. Kley. (2013). Modelling accretion in transitional disks. Springer Link (Chiba Institute of Technology). 11 indexed citations

Kley, W., et al.. (2013). The boundary layer in compact binaries. Springer Link (Chiba Institute of Technology). 10 indexed citations

10.

Kley, W., et al.. (2012). Low-mass planets in nearly inviscid disks: numerical treatment. Springer Link (Chiba Institute of Technology). 22 indexed citations

11.

Bitsch, Bertram & W. Kley. (2011). Evolution of inclined planets in three-dimensional radiative discs. Springer Link (Chiba Institute of Technology). 29 indexed citations

12.

Meru, Farzana, et al.. (2011). The four-population model: a new classification scheme for pre-planetesimal collisions. Springer Link (Chiba Institute of Technology). 18 indexed citations

13.

Rein, Hanno, J. C. B. Papaloizou, & W. Kley. (2010). The dynamical origin of the multi-planetary system HD 45364. Springer Link (Chiba Institute of Technology). 24 indexed citations

14.

Bitsch, B. & W. Kley. (2010). Orbital evolution of eccentric planets in radiative discs. Springer Link (Chiba Institute of Technology). 66 indexed citations

15.

Kuiper, R., Hubert Klahr, C. P. Dullemond, W. Kley, & Thomas Henning. (2010). Fast and accurate frequency-dependent radiation transport for hydrodynamics simulations in massive star formation. Springer Link (Chiba Institute of Technology). 84 indexed citations

16.

Kley, W., J. C. B. Papaloizou, & Gordon I. Ogilvie. (2008). Simulations of eccentric disks in close binary systems. Springer Link (Chiba Institute of Technology). 45 indexed citations

17.

Crida, A., Zs. Sándor, & W. Kley. (2008). Influence of an inner disc on the orbital evolution of massive planets migrating in resonance. Springer Link (Chiba Institute of Technology). 53 indexed citations

18.

Schäfer, Christoph, et al.. (2004). Evolution of irradiated circumbinary disks. Springer Link (Chiba Institute of Technology). 28 indexed citations

19.

Speith, R. & W. Kley. (2003). Stability of the viscously spreading ring. Springer Link (Chiba Institute of Technology). 12 indexed citations

20.

D’Angelo, Gennaro, Thomas Henning, & W. Kley. (2002). Nested-grid calculations of disk-planet interaction. Springer Link (Chiba Institute of Technology). 106 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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