N. D. Kee

628 total citations
22 papers, 307 citations indexed

About

N. D. Kee is a scholar working on Astronomy and Astrophysics, Molecular Biology and Fluid Flow and Transfer Processes. According to data from OpenAlex, N. D. Kee has authored 22 papers receiving a total of 307 indexed citations (citations by other indexed papers that have themselves been cited), including 22 papers in Astronomy and Astrophysics, 2 papers in Molecular Biology and 2 papers in Fluid Flow and Transfer Processes. Recurrent topics in N. D. Kee's work include Astrophysics and Star Formation Studies (20 papers), Stellar, planetary, and galactic studies (17 papers) and Astrophysical Phenomena and Observations (8 papers). N. D. Kee is often cited by papers focused on Astrophysics and Star Formation Studies (20 papers), Stellar, planetary, and galactic studies (17 papers) and Astrophysical Phenomena and Observations (8 papers). N. D. Kee collaborates with scholars based in United States, Belgium and Germany. N. D. Kee's co-authors include J. O. Sundqvist, S. P. Owocki, Asif ud‐Doula, R. Kuiper, J. Puls, I. El Mellah, Alexandre David-Uraz, G. A. Wade, L. Decin and H. Sana and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and The Astrophysical Journal Supplement Series.

In The Last Decade

N. D. Kee

19 papers receiving 271 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
N. D. Kee United States 11 290 55 24 15 13 22 307
Benjamin M. Tofflemire United States 12 280 1.0× 67 1.2× 15 0.6× 23 1.5× 9 0.7× 28 285
T. O. B. Schmidt Germany 15 492 1.7× 134 2.4× 15 0.6× 16 1.1× 19 1.5× 39 503
R. Petrucci Argentina 8 297 1.0× 132 2.4× 15 0.6× 10 0.7× 12 0.9× 9 304
D. Dimitrov Bulgaria 12 397 1.4× 133 2.4× 29 1.2× 11 0.7× 8 0.6× 35 406
F. Thévenin France 4 243 0.8× 144 2.6× 21 0.9× 12 0.8× 6 0.5× 4 248
Yuhiko Aoyama China 13 323 1.1× 30 0.5× 12 0.5× 10 0.7× 27 2.1× 25 331
Eric Stempels United States 8 349 1.2× 101 1.8× 7 0.3× 12 0.8× 14 1.1× 73 357
A. Milone Brazil 8 254 0.9× 118 2.1× 11 0.5× 25 1.7× 12 0.9× 17 268
Sarah Ballard United States 9 243 0.8× 95 1.7× 10 0.4× 9 0.6× 10 0.8× 26 247
D. T. Andreasen Portugal 8 213 0.7× 97 1.8× 19 0.8× 19 1.3× 10 0.8× 11 217

Countries citing papers authored by N. D. Kee

Since Specialization
Citations

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

Fields of papers citing papers by N. D. Kee

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by N. D. Kee. 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 N. D. Kee. The network helps show where N. D. Kee may publish in the future.

Co-authorship network of co-authors of N. D. Kee

This figure shows the co-authorship network connecting the top 25 collaborators of N. D. Kee. A scholar is included among the top collaborators of N. D. Kee 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 N. D. Kee. N. D. Kee 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
2.
Kee, N. D., et al.. (2024). Simulating the Photospheric to Coronal Plasma Using Magnetohydrodynamic Characteristics. I. Data-driven Boundary Conditions. The Astrophysical Journal Supplement Series. 270(2). 30–30. 9 indexed citations
3.
Kee, N. D. & R. Kuiper. (2022). Constraints on the stellar upper mass limit from simulations of UV disk ablation. Proceedings of the International Astronomical Union. 18(S361). 550–555.
4.
Kee, N. D., et al.. (2022). Method and new tabulations for flux-weighted line opacity and radiation line force in supersonic media. Astronomy and Astrophysics. 667. A113–A113. 9 indexed citations
5.
Sundqvist, J. O., et al.. (2022). First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds. Astronomy and Astrophysics. 665. A42–A42. 32 indexed citations
6.
Kee, N. D., J. O. Sundqvist, L. Decin, A. de Koter, & H. Sana. (2021). . UvA-DARE (University of Amsterdam). 1 indexed citations
7.
Sundqvist, J. O., N. D. Kee, S. P. Owocki, et al.. (2021). . UvA-DARE (University of Amsterdam). 23 indexed citations
8.
Kee, N. D., T. Shenar, J. Bodensteiner, et al.. (2021). Binary-object spectral-synthesis in 3D (BOSS-3D). Astronomy and Astrophysics. 660. A17–A17. 4 indexed citations
9.
Kee, N. D., et al.. (2021). Shock-heated radiation-driven outflows as a solution to the weak-wind problem of late O-type stars. Astronomy and Astrophysics. 648. A94–A94. 14 indexed citations
10.
Johnston, K., M. G. Hoare, H. Beuther, et al.. (2020). Spiral arms and instability within the AFGL 4176 mm1 disc. Astronomy and Astrophysics. 634. L11–L11. 32 indexed citations
11.
Kee, N. D., et al.. (2020). Line-drag damping of Alfvén waves in radiatively driven winds of magnetic massive stars. Monthly Notices of the Royal Astronomical Society. 499(3). 4282–4292. 2 indexed citations
12.
Puls, J., et al.. (2019). A 3D short-characteristics method for continuum and line scattering problems in the winds of hot stars. Springer Link (Chiba Institute of Technology). 11 indexed citations
13.
Sundqvist, J. O., et al.. (2019). Theoretical wind clumping predictions of OB supergiants from line-driven instability simulations across the bi-stability jump. Astronomy and Astrophysics. 631. A172–A172. 25 indexed citations
14.
Puls, J., et al.. (2018). 3D radiative transfer: Continuum and line scattering in non-spherical winds from OB stars. Springer Link (Chiba Institute of Technology). 15 indexed citations
15.
Kee, N. D., S. P. Owocki, & R. Kuiper. (2018). Line-driven ablation of circumstellar discs – III. Accountingfor and analysing the effects of continuum optical depth. Monthly Notices of the Royal Astronomical Society. 479(4). 4633–4641. 7 indexed citations
16.
ud‐Doula, Asif, S. P. Owocki, & N. D. Kee. (2018). Disruption of circumstellar discs by large-scale stellar magnetic fields. Monthly Notices of the Royal Astronomical Society. 478(3). 3049–3055. 19 indexed citations
17.
Kee, N. D., S. P. Owocki, & R. Kuiper. (2017). Line-driven ablation of circumstellar discs – II. Analysing the role of multiple resonances. Monthly Notices of the Royal Astronomical Society. 474(1). 847–853. 10 indexed citations
18.
David-Uraz, Alexandre, S. P. Owocki, G. A. Wade, J. O. Sundqvist, & N. D. Kee. (2017). Investigating the origin of cyclical wind variability in hot massive stars – II. Hydrodynamical simulations of corotating interaction regions using realistic spot parameters for the O giant ξ Persei. Monthly Notices of the Royal Astronomical Society. 470(3). 3672–3684. 19 indexed citations
19.
Kee, N. D., S. P. Owocki, & J. O. Sundqvist. (2016). Line-driven ablation of circumstellar discs – I. Optically thin decretion discs of classical Oe/Be stars. Monthly Notices of the Royal Astronomical Society. 458(3). 2323–2335. 37 indexed citations
20.
Kee, N. D., S. P. Owocki, & Asif ud‐Doula. (2014). Suppression of X-rays from radiative shocks by their thin-shell instability. Monthly Notices of the Royal Astronomical Society. 438(4). 3557–3567. 29 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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