P. Harmanec

2.2k total citations
132 papers, 914 citations indexed

About

P. Harmanec is a scholar working on Astronomy and Astrophysics, Instrumentation and Computational Mechanics. According to data from OpenAlex, P. Harmanec has authored 132 papers receiving a total of 914 indexed citations (citations by other indexed papers that have themselves been cited), including 120 papers in Astronomy and Astrophysics, 53 papers in Instrumentation and 31 papers in Computational Mechanics. Recurrent topics in P. Harmanec's work include Stellar, planetary, and galactic studies (105 papers), Astrophysics and Star Formation Studies (65 papers) and Astronomy and Astrophysical Research (53 papers). P. Harmanec is often cited by papers focused on Stellar, planetary, and galactic studies (105 papers), Astrophysics and Star Formation Studies (65 papers) and Astronomy and Astrophysical Research (53 papers). P. Harmanec collaborates with scholars based in Czechia, Canada and United States. P. Harmanec's co-authors include H. Božić, P. Koubský, M. Šlechta, S. Yang, M. Wolf, C. Aerts, Petr Škoda, P. Mayer, D. Sudar and A. Prša and has published in prestigious journals such as Nature, Science and The Astrophysical Journal.

In The Last Decade

P. Harmanec

119 papers receiving 886 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
P. Harmanec Czechia	17	884	280	72	29	24	132	914
Ε. N. Pastukhova Russia	11	631 0.7×	280 1.0×	101 1.4×	15 0.5×	17 0.7×	57	663
G. Cutispoto Italy	16	861 1.0×	198 0.7×	84 1.2×	16 0.6×	40 1.7×	72	879
Chun‐Hwey Kim South Korea	16	923 1.0×	290 1.0×	64 0.9×	32 1.1×	27 1.1×	65	950
Noel D. Richardson United States	15	719 0.8×	222 0.8×	53 0.7×	24 0.8×	34 1.4×	56	749
N. Vogt Chile	14	568 0.6×	111 0.4×	59 0.8×	25 0.9×	21 0.9×	74	582
F. Soydugan Türkiye	14	937 1.1×	350 1.3×	96 1.3×	23 0.8×	15 0.6×	61	947
D. Graczyk Poland	18	949 1.1×	449 1.6×	56 0.8×	30 1.0×	32 1.3×	58	989
H. F. Henrichs Netherlands	19	1.3k 1.4×	304 1.1×	115 1.6×	49 1.7×	24 1.0×	59	1.3k
A. Arellano Ferro Mexico	15	642 0.7×	360 1.3×	47 0.7×	8 0.3×	27 1.1×	88	667
E. Soydugan Türkiye	15	925 1.0×	364 1.3×	81 1.1×	27 0.9×	15 0.6×	46	933

Countries citing papers authored by P. Harmanec

Since Specialization

Citations

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

Fields of papers citing papers by P. Harmanec

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of P. Harmanec

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

Harmanec, P., P. Koubský, H. Božić, et al.. (2020). A new study of the spectroscopic binary 7 Vul with a Be star primary. Springer Link (Chiba Institute of Technology). 6 indexed citations

Harmanec, P., M. Brož, P. Mayer, et al.. (2017). Improved model of the triple system V746 Cassiopeiae that has a bipolar magnetic field associated with the tertiary. Springer Link (Chiba Institute of Technology). 1 indexed citations

Mayer, P., P. Harmanec, R. Chini, et al.. (2017). Physical properties of seven binary and higher-order multiple OB systems. Springer Link (Chiba Institute of Technology). 10 indexed citations

Harmanec, P., M. Wolf, H. Božić, et al.. (2014). Revised physical elements of the astrophysically important O9.5+O9.5V eclipsing binary system Y Cygni. Springer Link (Chiba Institute of Technology). 8 indexed citations

Johnston, C., E. F. Guinan, P. Harmanec, & P. Mayer. (2012). Demystifying the Confounding Long-Period Eclipsing Binary Epsilon Aurigae - Investigating Clues from its past behavior and possible Stellar Associates. AAS. 219.

Sudar, D., P. Harmanec, H. Lehmann, et al.. (2011). UX Monocerotis as a W Serpentis binary. Springer Link (Chiba Institute of Technology). 9 indexed citations

Harmanec, P., H. Božić, P. Mayer, et al.. (2011). V2368 Ophiuchi: an eclipsing and double-lined spectroscopic binary used as a photometric comparison star for U Ophiuchi. Springer Link (Chiba Institute of Technology). 1 indexed citations

Aerts, C., et al.. (2006). High-precision elements\nof double-lined spectroscopic binaries from combined\ninterferometry and spectroscopy. Springer Link (Chiba Institute of Technology). 10 indexed citations

Harmanec, P., J. Vondrák, P. Hadrava, et al.. (2006). The new orbital elements and properties of $\vec{\varepsilon}$ Persei. Astronomy and Astrophysics. 446(2). 583–589. 1 indexed citations

10.

Harmanec, P.. (2001). Hot emission-line stars after 134 years of study. A personal view of current problems. Digital Repository (National Repository of Grey Literature). 89. 9–22. 1 indexed citations

11.

Mayer, P., et al.. (1991). New Data on the Eclipsing Binary V1765 CYG (HR 7551) and Improved Orbital and Light-curve Solutions. Bulletin of the Astronomical Institutes of Czechoslovakia. 42. 230. 1 indexed citations

12.

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.

13.

Matthews, J. M., P. Harmanec, G. A. H. Walker, Shunfeng Yang, & W. H. Wehlau. (1990). A definitive period for the Be star LQ And.. JRASC. 84(6). 412. 1 indexed citations

14.

Harmanec, P.. (1988). Stellar masses and Radii based on modern binary data. Bulletin of the Astronomical Institutes of Czechoslovakia. 39(6). 329–345. 16 indexed citations

15.

Hubený, I., et al.. (1985). How Strong is the Evidence of Superionization and Large Mass Outflows in B/Be Stars?. Bulletin of the Astronomical Institutes of Czechoslovakia. 36(4). 214–230. 2 indexed citations

16.

Koubský, P., J. Horn, P. Harmanec, et al.. (1985). 96 Herculis: a remarkable early-type multiple system. Information Bulletin on Variable Stars. 2778. 1. 2 indexed citations

17.

Harmanec, P.. (1984). Re-Investigation of the Periodic and Long-Term Radial-Velocity Variations of the Be Star ζ Tau (HD 37202). Bulletin of the Astronomical Institutes of Czechoslovakia. 35(3). 164–179. 2 indexed citations

18.

Harmanec, P.. (1983). Review of observational facts about Be stars. 7(1). 55–88. 10 indexed citations

19.

Harmanec, P., et al.. (1972). The Shell Star 88 Herculis: Pulsating Envelope or Binary Star?. 11. 119. 1 indexed citations

20.

Plavec, M., et al.. (1968). EVOLUTION OF CLOSE BINARIES. I. TWO EXAMPLES OF MASS EXCHANGE IN PHASE I.. Bulletin of the Astronomical Institutes of Czechoslovakia. 19. 24. 1 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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