activity
20112018
most citedModified equipartition calculation for supernova remnants

57 citations · 104 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2018★ 12 cited

Searching for an interstellar medium association for HESS J1534-571

Nigel I. Maxted, C. Braiding, G. F. Wong +9

The Galactic supernova remnant HESS J1534-571 (also known as G323.7-1.0) has a shell-like morphology in TeV gamma-ray emission and is a key object in the study of cosmic ray origin…

astro-ph.GA2018★ 6 cited

A Multi-Frequency Study of the Milky Way-like Spiral Galaxy NGC 6744

Miranda Yew, Miroslav D. Filipović, Quentin Roper +14

We present a multi-frequency study of the intermediate spiral SAB(r)bc type galaxy NGC 6744, using available data from the Chandra X-Ray telescope, radio continuum data from the Au…

astro-ph.GA2015★ 3 cited

Optical observations of the nearby galaxy IC342 with narrow band [SII] and H filters. II - Detection of 16 Optically-Identified Supernova Remnant Candidates

M. M. Vucetic, A. Ciprijanovic, M. Z. Pavlovic +4

We present the detection of 16 optical supernova remnant (SNR) candidates in the nearby spiral galaxy IC342. The candidates were detected by applying [SII]/H ratio criterion on…

astro-ph.GA2013★ 3 cited

Optical observations of the nearby galaxy IC342 with narrow band [SII] and H filters. I

M. M. Vucetic, B. Arbutina, D. Urosevic +4

We present observations of the portion of the nearby spiral galaxy IC342 using narrow band [SII] and H filters. These observations were carried out in November 2011 with the 2m…

astro-ph.HE2013★ 23 cited

Modified equipartition calculation for supernova remnants. Cases α=0.5 and α=1

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

The equipartition or minimum-energy calculation is a well-known procedure for estimating magnetic field strength and total energy in the magnetic field and cosmic ray particles by…

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…