Abeona is confirmed as a faint ~30 arcmin bilateral radio SNR shell with synchrotron polarization, flux density 1.5 Jy, and a spatially coincident 5.7-sigma GeV gamma-ray source.
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2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.HE 2years
2026 2representative citing papers
Most cataloged Fermi point sources in the Vela region are spurious; the GeV emission is extended hadronic emission from the supernova remnant.
citing papers explorer
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Radio detection of supernova remnant G310.7-5.4 with $\gamma$-ray counterpart: Abeona SNR
Abeona is confirmed as a faint ~30 arcmin bilateral radio SNR shell with synchrotron polarization, flux density 1.5 Jy, and a spatially coincident 5.7-sigma GeV gamma-ray source.
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GeV emission in the region of Vela: a new view of the supernova remnant
Most cataloged Fermi point sources in the Vela region are spurious; the GeV emission is extended hadronic emission from the supernova remnant.