J1248+4826 is a newly identified compact ORC candidate with a ~30 kpc ring radius and ~200 kpc total extent at assumed z=0.2, consistent with the ORC population but with the host galaxy on the ring edge and no ongoing AGN activity.
Title resolution pending
4 Pith papers cite this work. Polarity classification is still indexing.
4
Pith papers citing it
representative citing papers
A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.
Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
citing papers explorer
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A Compact Radio Ring with a Diffuse Envelope in LOFAR: Odd Radio Circle or Distinct Phenomenon?
J1248+4826 is a newly identified compact ORC candidate with a ~30 kpc ring radius and ~200 kpc total extent at assumed z=0.2, consistent with the ORC population but with the host galaxy on the ring edge and no ongoing AGN activity.
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Discovery of a compact hierarchical triple main-sequence star system while searching for binary stars with compact objects
A new compact hierarchical triple main-sequence star system G1010 was discovered through combined low- and high-SNR spectroscopy, Gaia DR3 data, and TESS light curve analysis, showing an inner eclipsing binary rather than a compact object companion.
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Extending TESS flare frequency distributions with CHEOPS: Power-law versus lognormal
Combined TESS-CHEOPS data on 5620 flares shows ED-based FFDs follow power laws but bolometric-energy FFDs are best described by a truncated power law with break at 1.8e35 erg, with low-energy flattening attributed to detection biases rather than intrinsic lognormal behavior.
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Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.