activity
20062025
most citedStatistical Analysis of Supernova Remnants in the Large Magellanic Cloud

119 citations · 601 across the 43 of their papers we have counts for

collaborators

43 papers

astro-ph.SR2025

KIC 9272276: An Extreme Low Mass Ratio Red Nova Progenitor

Surjit Wadhwa, Marko Grozdanovic, Bojan Arbutina +2

Photometric analysis of KIC 9272276 (K9272), a low-mass contact binary system, is presented. We find it to be an example of an extreme low mass ratio system that satisfies the curr…

astro-ph.HE2025

Study of a giant Large Magellanic Cloud Supernova Remnant, Veliki (J0450.4-7050)

Z. J. Smeaton, M. D. Filipović, R. Z. E. Alsaberi +12

We present a high-resolution radio-continuum view and a multi-frequency analysis of the Large Magellanic Cloud (LMC) Supernova Remnant (SNR) J0450.4-7050, which we give the nicknam…

astro-ph.HE2024

Diprotodon on the sky. The Large Galactic Supernova Remnant (SNR) G278.94+1.35

Miroslav D. Filipović, S. Lazarević, M. Araya +41

We present a re-discovery of G278.94+1.35 as possibly one of the largest known Galactic supernova remnants (SNR) - that we name Diprotodon. While previously established as a Galact…

astro-ph.SR2024

Low Mass Contact Binaries: Orbital Stability at Extreme Low Mass Ratios

Surjit S. Wadhwa, Natalia R. Landin, Bojan Arbutina +5

With the ever-increasing number of light curve solutions of contact binary systems increasing number of potential bright red nova progenitors are being reported. There remains, how…

astro-ph.GA2024★ 2 cited

Supernova remnants in clumpy medium: A model of hydrodynamic and radio synchrotron evolution

Petar Kostić, Bojan Arbutina, Branislav Vukotić +1

We present an analytical model of relation for supernova remnants (SNRs) evolving in a clumpy medium. The model and its approximations were developed using the hydrodynamic s…

astro-ph.SR2024

The Critical Mass Ratio for W UMa-type Contact Binary Systems

Bojan Arbutina, Surjit Wadhwa

Contact binaries are close binary systems in which both components fill their inner Roche lobes so that the stars are in direct contact and in potential mass and energy exchange. T…