Б. Арбутина

591 total citations
35 papers, 368 citations indexed

About

Б. Арбутина is a scholar working on Astronomy and Astrophysics, Nuclear and High Energy Physics and Instrumentation. According to data from OpenAlex, Б. Арбутина has authored 35 papers receiving a total of 368 indexed citations (citations by other indexed papers that have themselves been cited), including 35 papers in Astronomy and Astrophysics, 20 papers in Nuclear and High Energy Physics and 6 papers in Instrumentation. Recurrent topics in Б. Арбутина's work include Astrophysics and Cosmic Phenomena (18 papers), Stellar, planetary, and galactic studies (15 papers) and Gamma-ray bursts and supernovae (14 papers). Б. Арбутина is often cited by papers focused on Astrophysics and Cosmic Phenomena (18 papers), Stellar, planetary, and galactic studies (15 papers) and Gamma-ray bursts and supernovae (14 papers). Б. Арбутина collaborates with scholars based in Serbia, Australia and Chile. Б. Арбутина's co-authors include D. Urošević, G. Djurašević, M. D. Filipović, N. F. H. Tothill, J. Petrović, Branislav Vukotić, S. O. Selam, B. Albayrak, A. Y. De Horta and D. Dimitrov and has published in prestigious journals such as The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society and Astronomy and Astrophysics.

In The Last Decade

Б. Арбутина

30 papers receiving 335 citations

Peers — A (Enhanced Table)

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

Name	h						Papers	Cites
Б. Арбутина Serbia	10	356	123	58	14	11	35	368
Iu. Babyk Ukraine	9	320 0.9×	108 0.9×	61 1.1×	10 0.7×	6 0.5×	34	330
Aleksey Generozov United States	10	356 1.0×	78 0.6×	40 0.7×	9 0.6×	14 1.3×	18	377
N. Lyskova Russia	10	244 0.7×	78 0.6×	95 1.6×	9 0.6×	8 0.7×	29	264
С. Н. Додонов Russia	11	312 0.9×	76 0.6×	73 1.3×	25 1.8×	11 1.0×	55	333
Firoza Sutaria India	12	261 0.7×	105 0.9×	49 0.8×	15 1.1×	14 1.3×	28	283
K. Azalee Bostroem United States	12	475 1.3×	91 0.7×	98 1.7×	12 0.9×	6 0.5×	36	488
P. M. Plewa Germany	7	296 0.8×	137 1.1×	21 0.4×	9 0.6×	26 2.4×	12	306
Sunmyon Chon Japan	10	337 0.9×	48 0.4×	93 1.6×	8 0.6×	8 0.7×	16	368
C. L. Bianco Italy	14	489 1.4×	169 1.4×	42 0.7×	17 1.2×	10 0.9×	67	509
Catherine Lovekin Canada	9	235 0.7×	51 0.4×	95 1.6×	30 2.1×	13 1.2×	24	274

Countries citing papers authored by Б. Арбутина

Since Specialization

Citations

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

Fields of papers citing papers by Б. Арбутина

Since Specialization

Physical SciencesHealth SciencesLife SciencesSocial Sciences

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

Co-authorship network of co-authors of Б. Арбутина

This figure shows the co-authorship network connecting the top 25 collaborators of Б. Арбутина. A scholar is included among the top collaborators of Б. Арбутина 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 Б. Арбутина. Б. Арбутина is excluded from the visualization to improve readability, since they are connected to all nodes in the network.

All Works

Sort: Min cites: Since: Top N: Style:

20 of 20 papers shown

Арбутина, Б., et al.. (2024). Supernova Remnants in Clumpy Medium: A Model of Hydrodynamic and Radio Synchrotron Evolution. The Astrophysical Journal. 974(2). 236–236.

Арбутина, Б., N. F. H. Tothill, A. Y. De Horta, et al.. (2024). Low-mass contact binaries: orbital stability at extreme low mass ratios. Monthly Notices of the Royal Astronomical Society. 535(3). 2494–2502. 2 indexed citations

Vince, O., Б. Арбутина, A. Y. De Horta, et al.. (2023). Effects of metallicity on the instability mass ratio of low-mass contact binary systems. Monthly Notices of the Royal Astronomical Society. 527(1). 1–9. 7 indexed citations

Арбутина, Б., J. Petrović, M. D. Filipović, et al.. (2023). A Study of Six Extreme Low Mass Ratio Contact Binary Systems. Publications of the Astronomical Society of the Pacific. 135(1051). 94201–94201. 3 indexed citations

Арбутина, Б.. (2023). Nonlinear diffusive shock acceleration of cosmic rays: quasi-thermal and non-thermal particle distributions. The European Physical Journal Plus. 138(9).

Арбутина, Б.. (2023). Diffusive Shock Acceleration of Cosmic Rays - Quasi-thermal and Non-thermal Particle Distributions. 31–31. 1 indexed citations

Арбутина, Б., N. F. H. Tothill, M. D. Filipović, et al.. (2023). A Study of Twelve Potential Merger Candidate Contact Binary Systems. Publications of the Astronomical Society of the Pacific. 135(1049). 74202–74202. 11 indexed citations

Horta, A. Y. De, M. D. Filipović, N. F. H. Tothill, et al.. (2022). Photometric Analysis of Three Potential Red Nova Progenitors. Research in Astronomy and Astrophysics. 22(10). 105009–105009. 9 indexed citations

Filipović, M. D., et al.. (2022). Simplified method for the identification of low mass ratio contact binary systems that are potential red nova progenitors. Journal of Astrophysics and Astronomy. 43(2). 7 indexed citations

10.

Filipović, M. D., et al.. (2020). ZZ Piscis Austrinus (ZZ PsA): a bright red nova progenitor and the instability mass ratio of contact binary stars. Monthly Notices of the Royal Astronomical Society. 501(1). 229–235. 51 indexed citations

11.

Ilić, D., Oleg V. Egorov, А. В. Моисеев, et al.. (2019). Revealing the nature of central emission nebulae in the dwarf galaxy NGC 185. Springer Link (Chiba Institute of Technology).

12.

Trčka, Ana, et al.. (2018). Optical observations of NGC 1156 galaxy in narrowband [SII] and Hα filters. Ghent University Academic Bibliography (Ghent University). 30(4). 379–386.

13.

Арбутина, Б., et al.. (2016). OPTICAL OBSERVATIONS OF THE NEARBY GALAXY IC342 WITH NARROW BAND [SII] AND Hα FILTERS. I∗. 2 indexed citations

14.

Арбутина, Б., et al.. (2014). Optical supernova remnants in nearby galaxies and their influence on star formation rates derived from Hα emission. Monthly Notices of the Royal Astronomical Society. 446(1). 943–958. 14 indexed citations

15.

Арбутина, Б.. (2012). The Minimum Mass Ratio for Contact Close Binary Systems of W Ursae Majoris-Type. 91. 391. 4 indexed citations

16.

Арбутина, Б., et al.. (2011). Numerical code for fitting radial emission profile of a shell supernova remnant: Application. Serbian Astronomical Journal. 77–85. 1 indexed citations

17.

Urošević, D., Branislav Vukotić, Б. Арбутина, et al.. (2009). The $\Sigma-{\sf \textit D}$ relation for planetary nebulae. Astronomy and Astrophysics. 495(2). 537–546. 4 indexed citations

18.

Арбутина, Б.. (2007). The minimum mass ratio of W UMa-type binary systems. Monthly Notices of the Royal Astronomical Society. 377(4). 1635–1637. 63 indexed citations

19.

Vukotić, Branislav, Б. Арбутина, & D. Ilić. (2007). THE Σ − D RELATION FOR PLANETARY NEBULAE: PRELIMINARY ANALYSIS. 2 indexed citations

20.

Djurašević, G., et al.. (2006). A Photometric Study of the Contact Binaries: XY Leo, EE Cet and AQ Psc. Publications of the Astronomical Society of Australia. 23(4). 154–164. 21 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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