collaborators

5 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

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…