At z=0.9, disk galaxies show a TFR slope of 3.82 and FR slope of 0.44 with moderate TFR and strong FR evolution from z=0, implying higher and less mass-dependent stellar-to-halo mass fractions f_M while f_j remains near 0.8.
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Sco-Cen shows abrupt jumps and plateaus in velocity dispersion correlated with star formation bursts, indicating isotropic expansion, inside-out propagation at 5-6 km/s, and stellar feedback as the primary driver.
Observational VLBI study of parsec-scale jets in 15 gamma-ray radio galaxies finds core flux density correlates with gamma-ray flux but gamma-ray luminosity shows no dependence on brightness temperature or core dominance.
The PRS of FRB 20190417A has a flat spectrum (α = 0.20) above 1 GHz with turnover >370 MHz, consistent with a magnetar wind nebula younger than 250 years and smaller than 0.4 pc.
PKS 0346-27 displayed a prolonged 2018 gamma-ray high state with ~1.5-hour variability, harder spectrum, and SED transition from LSP to ISP class, with one-zone leptonic modeling indicating lower magnetic field, larger radius, and higher electron energies than in quiescence.
citing papers explorer
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Kinematic scaling relations of disc galaxies from ionised gas at $z\sim1$ and their connection with dark matter haloes
At z=0.9, disk galaxies show a TFR slope of 3.82 and FR slope of 0.44 with moderate TFR and strong FR evolution from z=0, implying higher and less mass-dependent stellar-to-halo mass fractions f_M while f_j remains near 0.8.
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The evolution of velocity dispersion in the Sco-Cen OB association
Sco-Cen shows abrupt jumps and plateaus in velocity dispersion correlated with star formation bursts, indicating isotropic expansion, inside-out propagation at 5-6 km/s, and stellar feedback as the primary driver.
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Gamma-ray emission in radio galaxies under the VLBI scope -- I. Parsec-scale kinematics and high-energy properties of $\gamma$-ray detected TANAMI radio galaxies
Observational VLBI study of parsec-scale jets in 15 gamma-ray radio galaxies finds core flux density correlates with gamma-ray flux but gamma-ray luminosity shows no dependence on brightness temperature or core dominance.
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The spectrum of the persistent radio source associated with FRB 20190417A
The PRS of FRB 20190417A has a flat spectrum (α = 0.20) above 1 GHz with turnover >370 MHz, consistent with a magnetar wind nebula younger than 250 years and smaller than 0.4 pc.
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The large gamma-ray flare of the FSRQ PKS 0346-27
PKS 0346-27 displayed a prolonged 2018 gamma-ray high state with ~1.5-hour variability, harder spectrum, and SED transition from LSP to ISP class, with one-zone leptonic modeling indicating lower magnetic field, larger radius, and higher electron energies than in quiescence.