activity
20082019
most citedDiscovery of a Pulsar-powered Bow Shock Nebula in the Small Magellanic Cloud Supernova Remnant DEMS5

20 citations · 48 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019

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.GA20192 cited

Murchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1

D. Onić, M. D. Filipović, I. Bojičić +27

In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9+3.1. We present the radio spectral energy distr…

astro-ph.HE201920 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…

astro-ph.GA20195 cited

Optical observations of the nearby galaxy NGC 2366 through narrowband H and SII filters. Supernova remnants status

M. M. Vučetić, D. Onić, N. Petrov +2

We present detection of 67 HII regions and two optical supernova remnant (SNR) candidates in the nearby irregular galaxy NGC 2366. The SNR candidates were detected by applying [SII…

astro-ph.HE201516 cited

On the continuum radio-spectrum of Cas A: possible evidence of the non-linear particle acceleration

D. Onić, D. Urošević

Integrated radio-spectrum of Cas A in continuum was analyzed with special emphasis on possible high frequency spectral curvature. We conclude that the most probable scenario is tha…

astro-ph20085 cited

An analysis of the possible thermal emission at radio frequencies from an evolved supernova remnant HB 3 (G132.7 + 1.3): revisited

D. Onić, D. Urošević

It has recently been reported that some of the flux density values for an evolved supernova remnant (SNR) HB 3 (G132.7 + 1.3) are not accurate. In this work we revised an analysis…