2008/01/01 by E. J. Crawford, M. D. Filipović, J. L. Payne · 2 citations
Chemistry · Physics and Astronomy · #Astronomy #Astrophysics #Astrophysics and Cosmic Phenomena #Chemistry #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gamma-ray bursts and supernovae #Large Magellanic Cloud #Molecular cloud #Optics #Physics #Polarization (electrochemistry) #Stars #astro-ph
paper · pdf · doi:10.2298/saj0876059c
6 pages 4 figures, to be published in Serbian Astronomical Journal
openalex publication_date 2008/01/01 · arxiv created 2008/04/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We present the results of new high resolution ATCA observations of SNR J0519-6926. We found that this SNR exhibits a typical 'horseshoe' appearance with ?=-0.55?0.08 and D=28?1 pc. No polarization (or magnetic fields) were detected to a level of 1%. This is probably due to a relatively poor sampling of the UV plane caused be observing in 'snap-shot' mode.