activity
20232026
most citedThe role of impact parameter in typical close galaxy flybys

5 citations · 8 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

The habitability trade-off: Chemical decoupling and quenching in massive galaxies

Ana Mitrašinović, Nataša Pavlov, Branislav Vukotić +1

Massive galaxies experience complex evolutionary processes, including mergers and gas accretion, which can disrupt the chemical equilibrium between their stellar and gaseous compon…

astro-ph.GA2026

Puzzling Ultra-Diffuse Galaxy Evolution (PUDGE). II. A transformation pathway from ultra-diffuse galaxies to compact dwarfs in galaxy clusters

Nataša Pavlov, Ana Mitrašinović

Ultra-diffuse galaxies (UDGs) and compact dwarfs (CDs) occupy opposite extremes of the structural parameter space of dwarf galaxies, yet their spatial distributions in clusters sug…

astro-ph.GA2025

Discovery of a galaxy associated with the HI cloud FAST J0139+4328

Ana Mitrašinović, Marko Grozdanović, Ana Lalović +5

The search for ``dark galaxies,'' a key prediction of the lambda cold dark matter, has yielded few viable candidates. Recently, FAST J0139+4328 was reported as the first isolated d…

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

Galaxy Morphology Classification: Are Stellar Circularities Enough?

Katarina Baucalo, Ana Mitrašinović

We present a preliminary study exploring whether the stellar orbital circularity of simulated galaxies, available from precomputed catalogs in the IllustrisTNG project, can be used…

astro-ph.GA2025

Stealing galaxies from galaxy clusters

Majda Smole, Miroslav Micic, Ana Mitrašinović

We investigate galaxy groups that reside in the field but have been previously processed by galaxy clusters. Observationally, they would appear to have the same properties as regul…

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.GA2023

The isolated dark matter-poor galaxy that ran away. An example from IllustrisTNG

Ana Mitrašinović, Majda Smole, Miroslav Micic

Since the discovery of dark matter-deficient galaxies, numerous studies have shown that these exotic galaxies naturally occur in the CDM model due to stronger tidal interactions…

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…

astro-ph.GA2023★ 5 cited

The role of impact parameter in typical close galaxy flybys

A. Mitrašinović, M. Micic

Close galaxy flybys, interactions during which two galaxies inter-penetrate, are frequent and can significantly affect the evolution of individual galaxies. Equal-mass flybys are e…