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20062026
most citedStatistical Analysis of Supernova Remnants in the Large Magellanic Cloud

119 citations · 970 across the 55 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.GA2019★ 15 cited

Updated radio relation for Galactic supernova remnants -- II

B. Vukotić, A. Ćiprijanović, M. M. Vučetić +2

In this paper we present the updated empirical radio surface-brightness-to-diameter (--) relation for Galactic supernova remnants (SNRs) calibrated using SNRs with reli…

astro-ph.GA2019★ 32 cited

Radio Observations of Supernova Remnant G1.9+0.3

Kieran J. Luken, Miroslav D. Filipović, Nigel I. Maxted +18

We present 1 to 10GHz radio continuum flux density, spectral index, polarisation and Rotation Measure (RM) images of the youngest known Galactic Supernova Remnant (SNR) G1.9+0.3, u…

astro-ph.HE2019★ 12 cited

Radio Emission from Interstellar Shocks: Young Type Ia Supernova Remnants and the Case of N 103B in the Large Magellanic Cloud

R. Z. E. Alsaberi, L. A. Barnes, M. D. Filipovic +19

Here we present a radio continuum study based on new and archival data from the Australia Telescope Compact Array towards N 103B, a young (<=1000 yrs) spectroscopically confirmed t…

astro-ph.HE2019★ 9 cited

Particle acceleration in interstellar shocks

Dejan Urošević, Bojan Arbutina, Dušan Onić

This review presents the fundamentals of the particle acceleration processes active in interstellar medium (ISM), which are essentially based on the so-called Fermi mechanism theor…

astro-ph.GA2019★ 3 cited

Revealing the nature of central emission nebulae in the dwarf galaxy NGC 185

M. M. Vučetić, D. Ilić, O. V. Egorov +6

In this paper we present new optical observations of the galaxy NGC 185 intended to reveal the status of supernova remnants (SNRs) in this dwarf companion of the Andromeda galaxy.…

astro-ph.HE2019★ 20 cited

Discovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5

Rami Z. E. Alsaberi, C. Maitra, M. D. Filipovi'c +32

We report the discovery of a new Small Magellanic Cloud Pulsar Wind Nebula (PWN) at the edge of the Supernova Remnant (SNR)-DEM S5. The pulsar powered object has a cometary morphol…