А. Е. Тарасов

666 total citations
39 papers, 442 citations indexed

About

А. Е. Тарасов is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, А. Е. Тарасов has authored 39 papers receiving a total of 442 indexed citations (citations by other indexed papers that have themselves been cited), including 37 papers in Astronomy and Astrophysics, 10 papers in Instrumentation and 7 papers in Computational Mechanics. Recurrent topics in А. Е. Тарасов's work include Stellar, planetary, and galactic studies (25 papers), Astrophysics and Star Formation Studies (22 papers) and Astrophysical Phenomena and Observations (16 papers). А. Е. Тарасов is often cited by papers focused on Stellar, planetary, and galactic studies (25 papers), Astrophysics and Star Formation Studies (22 papers) and Astrophysical Phenomena and Observations (16 papers). А. Е. Тарасов collaborates with scholars based in Ukraine, Russia and United Kingdom. А. Е. Тарасов's co-authors include V. M. Lyuty, P. Roche, V. M. Larionov, C. Brocksopp, S. Rostopchin, J. Fabregat, J. S. Clark, M. J. Coe, P. F. Roche and R. P. Fender and has published in prestigious journals such as Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics and The Astronomical Journal.

In The Last Decade

А. Е. Тарасов

37 papers receiving 420 citations

Peers — A (Enhanced Table)

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

Name h Career Trend Papers Cites
А. Е. Тарасов Ukraine 11 431 75 54 40 33 39 442
F. Jablonski Brazil 12 456 1.1× 71 0.9× 62 1.1× 46 1.1× 48 1.5× 57 473
S. Yu. Shugarov Russia 10 352 0.8× 32 0.4× 48 0.9× 30 0.8× 57 1.7× 70 359
V. P. Goranskij Russia 11 316 0.7× 24 0.3× 65 1.2× 18 0.5× 45 1.4× 58 327
Н. А. Сахибуллин Russia 11 374 0.9× 44 0.6× 107 2.0× 25 0.6× 24 0.7× 51 385
Y. Tuchman Israel 10 290 0.7× 40 0.5× 71 1.3× 25 0.6× 21 0.6× 30 305
A. W. Woodsworth Canada 7 314 0.7× 76 1.0× 105 1.9× 17 0.4× 22 0.7× 22 342
R. Stehle Germany 12 380 0.9× 92 1.2× 17 0.3× 62 1.6× 14 0.4× 15 391
R. Zamanov Bulgaria 13 659 1.5× 128 1.7× 97 1.8× 60 1.5× 39 1.2× 59 670
P. Goldoni France 8 375 0.9× 108 1.4× 64 1.2× 15 0.4× 8 0.2× 25 392
R. González‐Riestra Spain 14 445 1.0× 103 1.4× 28 0.5× 38 0.9× 57 1.7× 37 459

Countries citing papers authored by А. Е. Тарасов

Since Specialization
Citations

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

Fields of papers citing papers by А. Е. Тарасов

Since Specialization
Physical SciencesHealth SciencesLife SciencesSocial Sciences

This network shows the impact of papers produced by А. Е. Тарасов. 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 А. Е. Тарасов. The network helps show where А. Е. Тарасов may publish in the future.

Co-authorship network of co-authors of А. Е. Тарасов

This figure shows the co-authorship network connecting the top 25 collaborators of А. Е. Тарасов. A scholar is included among the top collaborators of А. Е. Тарасов 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 А. Е. Тарасов. А. Е. Тарасов 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.
Тарасов, А. Е., et al.. (2012). Relative content of Be stars in young open star clusters. Astronomy Letters. 38(7). 428–435. 9 indexed citations
2.
Kim, Chulhee, A. V. Yushchenko, Ф. А. Мусаев, et al.. (2007). Chemical Composition and Differential Time-Series CCD Photometry of V2314 Ophiuchi: A New λ Bootis-Type Star. The Astronomical Journal. 134(3). 926–933. 3 indexed citations
3.
Lyuty, V. M., et al.. (2006). Long-Term Variations of the Supergiant in the X-Ray Binary Cyg X-1. IBVS. 5678. 1. 1 indexed citations
4.
Blay, P., I. Negueruela, P. Reig, et al.. (2006). Multiwavelength monitoring of BD +53°2790, the optical counterpart to 4U 2206+54. Astronomy and Astrophysics. 446(3). 1095–1105. 28 indexed citations
5.
Pogodin, M. A., А. С. Мирошниченко, А. Е. Тарасов, et al.. (2004). A new phase of activity of the Herbig Be star HD 200775 in2001: Evidence for binarity. Astronomy and Astrophysics. 417(2). 715–723. 16 indexed citations
6.
Yakut, K., А. Е. Тарасов, C. İbanoǧlu, et al.. (2003). Basic physical properties of the close binary V497 Cep in the open cluster NGC 7160. Astronomy and Astrophysics. 405(3). 1087–1093. 5 indexed citations
7.
Тарасов, А. Е., C. Brocksopp, & V. M. Lyuty. (2003). Variability of the Hα emission of Cygnus X-1 and its connection with the soft X-ray radiation. Astronomy and Astrophysics. 402(1). 237–246. 9 indexed citations
8.
Clark, J. S., et al.. (2003). Long term disc variability in the Be staroAndromedae. Astronomy and Astrophysics. 403(1). 239–246. 27 indexed citations
9.
Мирошниченко, А. С., J. Fabregat, K. S. Bjorkman, et al.. (2001). Spectroscopic observations of the δ Scorpii binary during its recent periastron passage. Astronomy and Astrophysics. 377(2). 485–495. 41 indexed citations
10.
Clark, J. S., А. Е. Тарасов, Atsuo T. Okazaki, P. Roche, & V. M. Lyuty. (2001). Phase changes of the Be/X-ray binary X Persei. Astronomy and Astrophysics. 380(2). 615–629. 30 indexed citations
11.
Тарасов, А. Е., S. V. Berdyugina, & A. Berdyugin. (1998). The massive interacting binary KX And: The orbit and physical parameters of the secondary component. Astronomy Letters. 24(3). 316–320. 2 indexed citations
12.
Berdyugin, A., S. V. Berdyugina, & А. Е. Тарасов. (1998). New photometric and polarimetric observations of the massive interacting binary KX And. Astronomy Letters. 24(3). 309–315. 1 indexed citations
13.
Rostopchin, S., et al.. (1998). The binary system V373 Cas: orbital elements, parameters of the components, and helium abundance. Astronomy Reports. 42(3). 312–321. 3 indexed citations
14.
Тарасов, А. Е., et al.. (1997). Photometric behavior of the binary system Cyg X-1/V1357 Cyg during the 1996 X-ray outburst. Astronomy Letters. 23(3). 293–298. 4 indexed citations
15.
Тарасов, А. Е., et al.. (1997). Long-term variability of the emission spectrum of the Be star β Cephei. Astronomy Letters. 23(4). 545–549. 7 indexed citations
16.
Rostopchin, S., et al.. (1995). The binary system alpha VIR (Spica) : fundamental parameters of the components and differences in their helium abundance.. Astronomicheskii Zhurnal. 39(2). 186–194. 1 indexed citations
17.
Тарасов, А. Е., P. Harmanec, S. Rostopchin, et al.. (1995). The archetype line-profile variable ∊ 45 Persei is a spectroscopic triple system.. 110. 59. 1 indexed citations
18.
Harmanec, P., Grant M. Hill, А. Е. Тарасов, et al.. (1991). Properties and nature of Be stars. XVI: Closer to a solution of the puzzle of 5 K Dra. Bulletin of the Astronomical Institutes of Czechoslovakia. 42(1). 39–61.
19.
Петров, П. П., et al.. (1985). The 1953-1984 Bright State of Ry-Tauri - Spectroscopy and Photometry. 11. 109. 1 indexed citations
20.
Петров, П. П., et al.. (1985). The 1983-1984 bright state of RY Tauri: Spectroscopy and photometry. Astronomy Letters. 11. 271–277. 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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