Б. Арбутина

University of Belgrade — RS

Physics and Astronomy · Physical Sciences

14h-index589citations106works1.52yr avg
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Research Topics

Astrophysics and Cosmic Phenomena(46), Gamma-ray bursts and supernovae(45), Stellar, planetary, and galactic studies(27), Radio Astronomy Observations and Technology(19), Solar and Space Plasma Dynamics(18)

Publications106 total

KIC 9272276: An Extreme Low Mass Ratio Red Nova Progenitor
arXiv (Cornell University)·2025Open Access
Study of a giant Large Magellanic Cloud Supernova Remnant, Veliki (J0450.4-7050)
arXiv (Cornell University)·2025Open Access
KIC 9272276: An extreme low mass ratio red nova progenitor
Serbian Astronomical Journal·2025Open Access
Study of a giant large Magellanic Cloud Supernova Remnant, Veliki (J0450.4-7050)
Serbian Astronomical Journal·2025Open Access
Diprotodon on the sky. The Large Galactic Supernova Remnant (SNR) G278.94+1.35
arXiv (Cornell University)·2024Open Access
THE LIFE AND WORK OF ELIA MILLOSEVICH (1848-1919)
2024Open Access
SERBIAN ASTRONOMICAL JOURNAL IN THE 2003-2023 PERIOD
2024Open Access
ASTRONOMY EDUCATION IN SERBIA 2020-2023
2024Open Access
HYDRODYNAMIC SIMULATIONS OF SUPERNOVA REMNANTS ENCOUNTERING HIGH DENSITY ENVIRONMENT
2024Open Access
ON THE ORIGIN OF THE NORTH POLAR SPUR
2024Open Access
THE CRITICAL MASS RATIO FOR W UMA-TYPE CONTACT BINARIES
2024Open Access
Low-mass contact binaries: orbital stability at extreme low mass ratios
Monthly Notices of the Royal Astronomical Society·2024· 7 citedOpen Access
Low Mass Contact Binaries: Orbital Stability at Extreme Low Mass Ratios
arXiv (Cornell University)·2024Open Access
Supernova Remnants in Clumpy Medium: A Model of Hydrodynamic and Radio Synchrotron Evolution
The Astrophysical Journal·2024· 2 citedOpen Access
The Critical Mass Ratio for W UMa-type Contact Binary Systems
arXiv (Cornell University)·2024Open Access
Diprotodon on the sky. The Large Galactic Supernova Remnant (SNR) G278.94+1.35
Publications of the Astronomical Society of Australia·2024· 2 citedOpen Access
Erratum: The critical mass ratio for W UMa-type contact binary systems (Serb. Astron. J. No. 208 (2024), 1)
Serbian Astronomical Journal·2024Open Access
The critical mass ratio for W UMa-type contact binary systems
Serbian Astronomical Journal·2024· 16 citedOpen Access
Effects of metallicity on the instability mass ratio of low-mass contact binary systems
Monthly Notices of the Royal Astronomical Society·2023· 9 citedOpen Access
Effects of Metallicity on the Instability Mass Ratio of Low Mass Contact Binary Systems
arXiv (Cornell University)·2023Open Access
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Frequent Co-authors

D. Urošević(24), M. D. Filipović(15), Surjit S. Wadhwa(12), Branislav Vukotić(12), N. F. H. Tothill(10), J. Petrović(10), G. Djurašević(10), A. Y. De Horta(8), Marko Z. Pavlović(7), M. M. Vučetić(6), N. Hurley‐Walker(4), Gavin Rowell(4), M. Andjelić(3), Shi Dai(3), Robert Brose(3), Hidetoshi Sano(3), T. H. Jarrett(3), R. Z. E. Alsaberi(3), Cristóbal Bordiú(3), F. Bufano(3)