activity
20062025
most citedThe radio surface brightness to diameter relation for galactic supernova remnants: sample selection and robust analysis with various fitting offsets

89 citations · 519 across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.GA2025★ 2 cited

Orientation of galaxy spins relative to filaments of the large-scale structure of the Universe

A. V. Antipova, D. I. Makarov, N. Libeskind +1

The theory of galaxy formation posits a clear correlation between the spin of galaxies and the orientation of the elements of the large-scale structure of the Universe, particularl…

astro-ph.GA2025★ 1 cited

Revisiting the bimodality of galactic habitability in IllustrisTNG

Ana Mitrašinović, Branislav Vukotić, Teodora Žižak +2

The potential of galaxies to host habitable planets is central to astrobiology, tightly linked to galaxy-scale evolution and cosmological processes. Using IllustrisTNG, we revisit…

astro-ph.HE2025

Teleios (G305.4-2.2) -- the mystery of a perfectly shaped new Galactic supernova remnant

Miroslav D. Filipovic, Zachary J. Smeaton, Roland Kothes +35

We present the serendipitous radio-continuum discovery of a likely Galactic supernova remnant (SNR) G305.4-2.2. This object displays a remarkable circular symmetry in shape, making…

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.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.GA2023

Dynamical aspects of Galactic habitability in N-body simulations

A. Mitrašinović, B. Vukotić, M. Micic +1

Recent studies of Galactic evolution revealed that the dynamics of the stellar component might be one of the key factors when considering galactic habitability. We run an N-body si…