Yet another Odd Radio Circle?
arXiv:2205.08092 · doi:10.3847/2515-5172/ac7044
Abstract
The Odd Radio Circles are newly identified diffuse radio sources at ~1 GHz frequency, with edge-brightened nearly circular morphology, which is remarkably similar to supernova remnants although a physical association with previous population of Galactic supernova remnants is challenging due to detections of the Odd Radio Circles at high Galactic latitudes. Here, a serendipitous identification of a new source in a LOFAR 144 MHz image with similar morphology as that of Odd Radio Circles is reported. This is the first reported identification of an Odd Radio Circle at a very low frequency and with the LOFAR.
arXiv comment5 pages, 1 figure, Accepted in RNAAS
References in corpus (7)
- The Pan-STARRS1 Database and Data Products
- The LOFAR Two-metre Sky Survey -- V. Second data release
- Unexpected Circular Radio Objects at High Galactic Latitude
- MeerKAT uncovers the physics of an Odd Radio Circle
- Unveiling the rarest morphologies of the LOFAR Two-metre Sky Survey radio source population with self-organised maps
- Mysterious Odd Radio Circle near the Large Magellanic Cloud -- An Intergalactic Supernova Remnant?
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Cited by in corpus (5)
- Insights on the origin of ORCs from cosmological simulations
- Discovery of a circularly symmetric extended diffuse radio emission around an elliptical galaxy with the VLA FIRST survey
- On energetics and progenitors of Odd Radio Circles: A causal connection with tidal disruption of stars?
- Discovery of Odd Radio Circles and Other Peculiars in the First Year of the EMU Survey using Object Detection
- Circular Mystery: Exploring Diffuse Emission Surrounding a Radio Galaxy with uGMRT and VLA Multiwavelength Observations