First VLTI-GRAVITY near-infrared observations of blazars indicate possible detection of unresolved or partially resolved jet emission in Ton 599, though data cannot distinguish extended structure from instrumental coherence loss.
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GRB 210704A at z=2.34 shows a luminous fast blue transient excess peaking at ~7 days, modeled as refreshed shock emission and linked to LFBOTs alongside a high-Lorentz-factor jet.
No significant environmental dependence is found for the galaxy size-mass relation at low redshift across clusters, voids, cluster masses, and cluster-centric distances.
Cool gas inflows occur in ~70% of red geyser galaxies at median 47 km/s, with reservoirs 7 times larger in radio-detected systems and 2.7 times larger in interacting ones, linking galaxy environment to AGN fueling and quiescence regulation.
New XMM-Newton data on MCG+11--11--032 shows no double Fe Kα line, inconsistent with a binary black hole candidate and consistent with a single AGN.
citing papers explorer
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VLTI-GRAVITY observations of blazars
First VLTI-GRAVITY near-infrared observations of blazars indicate possible detection of unresolved or partially resolved jet emission in Ton 599, though data cannot distinguish extended structure from instrumental coherence loss.
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GRB 210704A: A Luminous Fast Blue Transient in a GRB Afterglow at $z = 2.34$
GRB 210704A at z=2.34 shows a luminous fast blue transient excess peaking at ~7 days, modeled as refreshed shock emission and linked to LFBOTs alongside a high-Lorentz-factor jet.
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From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift
No significant environmental dependence is found for the galaxy size-mass relation at low redshift across clusters, voids, cluster masses, and cluster-centric distances.
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Galactic Rain: Cool Gas Inflows in Red Geyser Galaxies and Their Connection to AGN Activity and Interactions
Cool gas inflows occur in ~70% of red geyser galaxies at median 47 km/s, with reservoirs 7 times larger in radio-detected systems and 2.7 times larger in interacting ones, linking galaxy environment to AGN fueling and quiescence regulation.
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An XMM-Newton Analysis of the Supermassive Black Hole Binary Candidate MCG+11--11--032
New XMM-Newton data on MCG+11--11--032 shows no double Fe Kα line, inconsistent with a binary black hole candidate and consistent with a single AGN.