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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 2011Show all

6 papers · 1 filter

astro-ph.CO2011★ 1 cited

Observatons of NGC 3077 Galaxy in Narrow Band [SII] and H_alpha Filters

M. Andjelic, K. Stavrev, B. Arbutina +2

We present observations of the HI tidal arm near dwarf galaxy NGC 3077 (member of the M81 galaxy group) in narrow band [SII] and H_alpha filters. Observations were carried out in M…

astro-ph.HE2011★ 28 cited

Multi-frequency study of the Large Magellanic Cloud Supernova Remnant J0529-6653 near Pulsar B0529-66

L. M. Bozzetto, M. D. Filipović, E. J. Crawford +11

We report the ATCA and ROSAT detection of Supernova Remnant (SNR) J0529--6653 in the Large Magellanic Cloud (LMC) which is positioned in the projected vicinity of the known radio p…

astro-ph.HE2011★ 57 cited

Modified equipartition calculation for supernova remnants

B. Arbutina, D. Urosevic, M. M. Andjelic +2

Determination of the magnetic field strength in the interstellar medium is one of the most complex tasks of contemporary astrophysics. We can only estimate the order of magnitude o…

astro-ph.GA2011

Spectra of HB 21 supernova remnant: Evidence of spectra flattening at the low frequencies

D. Borka, V. Borka Jovanović, D. Urošević

We use observations of the continuum radio emission at 1420, 820, 408, 34.5 and 22 MHz to estimate the mean brightness temperatures of the HB 21 supernova remnant (SNR) at five fre…

astro-ph.GA2011

The brightness temperatures of the main Galactic radio-loops at 22 MHz

D. Urošević, V. Borka Jovanović

The average brightness temperatures and surface brightnesses at 22 MHz are derived for the four main Galactic radio-continuum loops (Loops I, II, III and IV, hereafter radio-loops)…

astro-ph.GA2011★ 1 cited

Temperature, brightness and spectral index of the Cygnus radio loop

V. Borka Jovanović, D. Urošević

The estimated brightness of the Cygnus loop supernova remnant (SNR) at 2720, 1420, 820, 408 and 34.5 MHz are presented. The observations of the continuum radio emission are used to…