SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.
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3 Pith papers cite this work, alongside 32 external citations. Polarity classification is still indexing.
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2026 3representative citing papers
CSO-2 radio lobes sit near minimum-energy magnetic fields of ~20 mG, implying rapid GHz fading post-jet-shutoff and massive-star origins for luminous sources.
Including radiative losses in analytic models of high-redshift radio galaxies reduces predicted radio and X-ray luminosities compared to models that neglect them.
citing papers explorer
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SDSSJ110546.07+145202.4: The first long-duration radio changing-look NLS1 galaxy
SDSSJ110546.07+145202.4 is the first known long-duration radio changing-look NLS1 galaxy whose outburst is explained by an accretion-rate change that triggered a powerful radio jet.
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Minimum Energies and Magnetic Field Strengths of Edge-brightened Compact Symmetric Objects
CSO-2 radio lobes sit near minimum-energy magnetic fields of ~20 mG, implying rapid GHz fading post-jet-shutoff and massive-star origins for luminous sources.
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A simulation-based analytic model of radio galaxies II: self-consistent radiative losses
Including radiative losses in analytic models of high-redshift radio galaxies reduces predicted radio and X-ray luminosities compared to models that neglect them.