T. Nakamoto

2.1k total citations
63 papers, 1.4k citations indexed

About

T. Nakamoto is a scholar working on Astronomy and Astrophysics, Spectroscopy and Materials Chemistry. According to data from OpenAlex, T. Nakamoto has authored 63 papers receiving a total of 1.4k indexed citations (citations by other indexed papers that have themselves been cited), including 41 papers in Astronomy and Astrophysics, 11 papers in Spectroscopy and 10 papers in Materials Chemistry. Recurrent topics in T. Nakamoto's work include Astrophysics and Star Formation Studies (29 papers), Astro and Planetary Science (25 papers) and Stellar, planetary, and galactic studies (14 papers). T. Nakamoto is often cited by papers focused on Astrophysics and Star Formation Studies (29 papers), Astro and Planetary Science (25 papers) and Stellar, planetary, and galactic studies (14 papers). T. Nakamoto collaborates with scholars based in Japan, United States and Russia. T. Nakamoto's co-authors include Masao Mori, Shin Mineshige, Ken Ohsuga, Hajime Susa, Hitoshi Miura, Masayuki Umemura, Shigeru Ida, Hiroyuki Kurokawa, Hidekazu Tanaka and Yui Kawashima and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Journal of the Atmospheric Sciences.

In The Last Decade

T. Nakamoto

61 papers receiving 1.3k citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
T. Nakamoto Japan 17 1.3k 171 137 110 102 63 1.4k
H. P. Gail Germany 26 2.0k 1.6× 76 0.4× 204 1.5× 295 2.7× 170 1.7× 86 2.3k
Akemi Tamanai Germany 17 1.7k 1.4× 70 0.4× 141 1.0× 89 0.8× 121 1.2× 31 2.0k
A. Evans United Kingdom 26 2.2k 1.7× 350 2.0× 85 0.6× 170 1.5× 68 0.7× 177 2.3k
J. Dorschner Germany 20 1.7k 1.4× 55 0.3× 161 1.2× 219 2.0× 224 2.2× 90 2.0k
B. M. Swinyard United Kingdom 22 1.4k 1.1× 199 1.2× 373 2.7× 13 0.1× 287 2.8× 111 1.7k
K.‐P. Schröder Mexico 21 1.7k 1.3× 108 0.6× 49 0.4× 37 0.3× 49 0.5× 58 1.8k
Takayoshi Sano Japan 23 1.2k 0.9× 469 2.7× 117 0.9× 323 2.9× 43 0.4× 99 1.8k
C. D. Dowell United States 28 2.5k 2.0× 341 2.0× 264 1.9× 41 0.4× 184 1.8× 98 2.7k
J. S. Greaves United Kingdom 31 3.1k 2.4× 257 1.5× 236 1.7× 54 0.5× 145 1.4× 99 3.2k
A. K. Speck United States 22 1.2k 0.9× 64 0.4× 87 0.6× 123 1.1× 84 0.8× 69 1.4k

Countries citing papers authored by T. Nakamoto

Since Specialization
Citations

This map shows the geographic impact of T. Nakamoto'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 T. Nakamoto with the expected number of citations based on a country's size and research output (numbers larger than one mean the country cites T. Nakamoto more than expected).

Fields of papers citing papers by T. Nakamoto

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of T. Nakamoto

This figure shows the co-authorship network connecting the top 25 collaborators of T. Nakamoto. A scholar is included among the top collaborators of T. Nakamoto 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 T. Nakamoto. T. Nakamoto 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.
Okuzumi, Satoshi, Hidekazu Tanaka, Eiichiro Kokubo, et al.. (2023). Size Dependence of the Bouncing Barrier in Protoplanetary Dust Growth. The Astrophysical Journal Letters. 951(1). L16–L16. 14 indexed citations
2.
Yamamoto, Daiki, T. Ushikubo, H. Kaneko, et al.. (2023). Oxygen isotope exchange between molten silicate spherules and ambient water vapor with nonzero relative velocity: Implication for chondrule formation environment. Icarus. 405. 115690–115690. 1 indexed citations
3.
Nomura, Hideko, Aya E. Higuchi, Nami Sakai, et al.. (2018). ALMA observations of sulfur-bearing molecules in protoplanetary disks. Proceedings of the International Astronomical Union. 14(S345). 360–361. 1 indexed citations
4.
Miura, Hitoshi, Tetsuo Yamamoto, Hideko Nomura, et al.. (2017). Comprehensive Study of Thermal Desorption of Grain-surface Species by Accretion Shocks around Protostars. The Astrophysical Journal. 839(1). 47–47. 23 indexed citations
5.
6.
Tanaka, Kyoko K., Tetsuo Yamamoto, Hidekazu Tanaka, et al.. (2013). EVAPORATION OF ICY PLANETESIMALS DUE TO BOW SHOCKS. The Astrophysical Journal. 764(2). 120–120. 11 indexed citations
7.
Inoue, Akio, et al.. (2012). EFFECT OF PHOTODESORPTION ON THE SNOW LINES AT THE SURFACE OF OPTICALLY THICK CIRCUMSTELLAR DISKS AROUND HERBIG Ae/Be STARS. The Astrophysical Journal. 747(2). 138–138. 10 indexed citations
8.
Nakamoto, T. & Keisuke Murakami. (2009). Selection Method of Odor Components for Olfactory Display Using Mass Spectrum Database. 159–162. 13 indexed citations
9.
Yajima, Hidenobu, Masayuki Umemura, Masao Mori, & T. Nakamoto. (2009). The escape of ionizing photons from supernova-dominated primordial galaxies. Monthly Notices of the Royal Astronomical Society. 398(2). 715–721. 37 indexed citations
10.
Miura, Hitoshi & T. Nakamoto. (2007). Shock-wave heating model for chondrule formation: Hydrodynamic simulation of molten droplets exposed to gas flows. Icarus. 188(1). 246–265. 10 indexed citations
11.
Yasuda, Seiji & T. Nakamoto. (2006). Possible Size of Porphyritic Chondrules in Shock-Wave Heating Model. LPI. 1674. 2 indexed citations
12.
Iliev, Ilian T., B. Ciardi, Marcelo A. Alvarez, et al.. (2006). Cosmological radiative transfer codes comparison project ��� I. The static density field tests. Monthly Notices of the Royal Astronomical Society. 371(3). 1057–1086. 150 indexed citations
13.
Miura, Hitoshi & T. Nakamoto. (2005). Appropriate Shock Waves for Chondrule Formation: Heating Rate and Cooling Rate Constraints. 36th Annual Lunar and Planetary Science Conference. 1248. 1 indexed citations
14.
Desch, S. J., F. J. Ciesla, L. L. Hood, & T. Nakamoto. (2005). Heating of Chondritic Materials in Solar Nebula Shocks. ASPC. 341. 849. 35 indexed citations
15.
Nakamoto, T., N. T. Kita, & Shogo Tachibana. (2005). Chondrule age distribution and rate of heating events for chondrule formation. Institutional Repository National Institute of Polar Research (National Institute of Polar Research (Japan)). 18. 253–272. 2 indexed citations
16.
Miura, Hitoshi & T. Nakamoto. (2005). Thermal history of chondrules during shock-wave heating. Institutional Repository National Institute of Polar Research (National Institute of Polar Research (Japan)). 18. 239–252. 1 indexed citations
17.
Nakamoto, T., M. Hayashi, N. T. Kita, & Shogo Tachibana. (2004). Chondrule Forming Shock Waves in Solar Nebula by X-Ray Flares. ASPC. 341. 883. 7 indexed citations
18.
Nakamoto, T. & Hitoshi Miura. (2004). Collisional Destruction of Chondrules in Shock Waves and Inferred Dust to Gas Mass Ratio. Lunar and Planetary Science Conference. 1847. 6 indexed citations
19.
Nakamoto, T., et al.. (1994). Mössbauer spectroscopic studies on mixed-valence states in trinuclear iron carboxylates. Hyperfine Interactions. 84(1). 589–594. 6 indexed citations
20.

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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