A low-luminosity AGN in ESO 420-G13 powers a jet-driven gas bubble and massive CO-dark molecular outflow with total kinetic power ~1.5e41 erg/s and ~3.8% coupling efficiency, expelling ~5% of the central molecular gas.
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5 Pith papers cite this work. Polarity classification is still indexing.
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EPTA second data release reports Bayes factor of 60 for an isotropic nanohertz GWB in the 10.3-year subset, with amplitude (2.5±0.7)×10^{-15} at 1 yr^{-1} when spectral index is fixed at 13/3.
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
A catalog of 6104 high-redshift quasar candidates (4.5 < z < 7) in the southern hemisphere was produced via multiwavelength photometry and SED fitting, with spectroscopic confirmation of three objects at z > 5.
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.
citing papers explorer
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Wild is the wind from low-luminosity AGN: a jet-driven gas bubble blowing out a massive CO-dark outflow in ESO 420-G13
A low-luminosity AGN in ESO 420-G13 powers a jet-driven gas bubble and massive CO-dark molecular outflow with total kinetic power ~1.5e41 erg/s and ~3.8% coupling efficiency, expelling ~5% of the central molecular gas.
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The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
EPTA second data release reports Bayes factor of 60 for an isotropic nanohertz GWB in the 10.3-year subset, with amplitude (2.5±0.7)×10^{-15} at 1 yr^{-1} when spectral index is fixed at 13/3.
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Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
Outliers from the black hole-stellar mass scaling relation arise from distinct channels of enhanced mergers with super-Eddington growth, gravitational recoils after mergers, environmental stellar mass loss, and quiescent histories.
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4MOST ChANGES: Catalog of high-redshift quasar candidates (4.5 < $z$ < 7) selected with SED fitting
A catalog of 6104 high-redshift quasar candidates (4.5 < z < 7) in the southern hemisphere was produced via multiwavelength photometry and SED fitting, with spectroscopic confirmation of three objects at z > 5.
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What Does the Virial Coefficient of the \Hb Broad-Line Region Depend On?
Recovers individual f virial factors from dynamical modeling plus RM data and reports evidence for correlation of log f with black hole mass plus marginal links to BLR thickness, inclination, and line shape.