Detection of a time-variable relativistic UV outflow at velocities up to 0.3c in quasar J2318, with estimated mass-loss rate and kinetic luminosity above typical feedback thresholds.
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The W cloud is reinterpreted as a disrupting galaxy group with a dynamically coherent tidal tail delivering low-mass star-forming dwarfs to the Virgo cluster.
CLUMI+ jointly models weak and strong lensing with caustic escape-velocity data, recovering cluster mass profiles from core to infall without equilibrium assumptions.
Using 11 CLASH clusters, this paper finds that satellite quenching is anisotropic out to at least 2.5 R200, peaking near 1.25 R200, and concludes pre-processing in large-scale structure, not AGN feedback, drives the signal.
SDSS J121929.45+471522.8 is found to be the third isolated magnetic white dwarf with Zeeman-split Balmer emission, closely matching the other two known cases.
Four Planck-selected dusty star-forming galaxies are confirmed as strongly lensed at z≈2.3–3.3 via NOEMA CO line detections; a lens model for one source yields µ≈11.
A new Python tool and template set show that the 40 km/s SDSS versus Hectospec redshift offset is caused by template velocity offsets, and calibrating templates to synthetic rest-frame spectra removes the offset.
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A New Member of the Fast and Furious Family: A Relativistic and Time-Variable UV Outflow in a Luminous Quasar
Detection of a time-variable relativistic UV outflow at velocities up to 0.3c in quasar J2318, with estimated mass-loss rate and kinetic luminosity above typical feedback thresholds.
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Hierarchical assembly in action: a galaxy tail from a disrupting group in the Virgo cluster outskirts
The W cloud is reinterpreted as a disrupting galaxy group with a dynamically coherent tidal tail delivering low-mass star-forming dwarfs to the Virgo cluster.