Statistical analysis of supernova remnants in the Large Magellanic Cloud

LM Bozzetto, MD Filipović, B Vukotić… - The Astrophysical …, 2017 - iopscience.iop.org
We construct the most complete sample of supernova remnants (SNRs) in any galaxy—the
Large Magellanic Cloud (LMC) SNR sample. We study their various properties such as …

Constraints on the distribution of supernova remnants with Galactocentric radius

DA Green - Monthly Notices of the Royal Astronomical Society, 2015 - academic.oup.com
Supernova remnants (SNRs) in the Galaxy are an important source of energy injection into
the interstellar medium, and also of cosmic rays. Currently there are 294 known SNRs in the …

On the Determination of the Evolutionary Status of Supernova Remnants from Radio Observation Data

D Urošević - Publications of the Astronomical Society of the …, 2022 - iopscience.iop.org
This paper aims to give a brief review of a new concept for the preliminary determination of
the evolutionary status of supernova remnants (SNRs). Data obtained by radio observations …

The radio surface-brightness-to-diameter relation for Galactic supernova remnants: sample selection and robust analysis with various fitting offsets

MZ Pavlović, D Urošević, B Vukotić… - The Astrophysical …, 2012 - iopscience.iop.org
In this paper, we present new empirical radio surface-brightness-to-diameter (Σ–D) relations
for supernova remnants (SNRs) in our Galaxy. We also present new theoretical derivations …

Updated radio relation for Galactic supernova remnants

MZ Pavlović, A Dobardžić, B Vukotić… - arXiv preprint arXiv …, 2014 - arxiv.org
We present updated empirical radio surface-brightness-to-diameter ($\Sigma-D $) relation
for supernova remnants (SNRs) in our Galaxy. Our original calibration sample of Galactic …

Radio evolution of supernova remnants including nonlinear particle acceleration: insights from hydrodynamic simulations

MZ Pavlović, D Urošević, B Arbutina… - The Astrophysical …, 2018 - iopscience.iop.org
We present a model for the radio evolution of supernova remnants (SNRs) obtained by
using three-dimensional hydrodynamic simulations coupled with nonlinear kinetic theory of …

SRG/eROSITA discovery of a large circular SNR candidate G116.6−26.1: SN Ia explosion probing the gas of the Milky Way halo?

EM Churazov, II Khabibullin, AM Bykov… - Monthly Notices of …, 2021 - academic.oup.com
We report a discovery of a new X-ray-selected supernova remnant (SNR) candidate SRGe
J0023+ 3625= G116. 6− 26.1 found in the SRG/eROSITA all-sky survey. The source features …

SXP 1062, a young Be X-ray binary pulsar with long spin period-Implications for the neutron star birth spin

F Haberl, R Sturm, MD Filipović, W Pietsch… - Astronomy & …, 2012 - aanda.org
Context. The Small Magellanic Cloud (SMC) is ideally suited to investigating the recent star
formation history from X-ray source population studies. It harbours a large number of Be/X …

[PDF][PDF] The influence of supernova remnants on the interstellar medium in the Large Magellanic Cloud seen at 20–600 µm wavelengths

M Lakicevic, JT Van Loon, M Meixner, K Gordon… - arXiv preprint arXiv …, 2014 - Citeseer
We present the analysis of supernova remnants (SNRs) in the Large Magellanic Cloud
(LMC) and their influence on the environment at far-infrared (FIR) and submillimeter …

SRG/eROSITA discovery of a radio-faint X-ray candidate supernova remnant SRGe J003602.3+605421 = G121.1−1.9

II Khabibullin, EM Churazov, AM Bykov… - Monthly Notices of …, 2023 - academic.oup.com
We report the discovery of a candidate X-ray supernova remnant SRGe J003602. 3+
605421= G121. 1− 1.9 in the course of the SRG/eROSITA all-sky survey. The object is …