3D MHD simulations show high-thrust, magnetically stabilized jets reach 5 Mpc in 15 Myr while weaker jets disrupt at ~3 Mpc over 35 Myr.
The Astrophysical Journal , archivePrefix = "arXiv", eprint =
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X-ray detection of M~1.3 merger shock in A2142, reproduced by off-axis merger simulations, with radio arcs interpreted as shock-induced vortex rings and ultra-long tails explained by post-shock electron re-acceleration and plasma stretching.
FRB dispersion measures directly constrain suppression of the matter power spectrum due to feedback at k ~ 0.1-3 h/Mpc, reduce posterior variance by a factor of ~8 at k~1 h/Mpc, and exclude extreme large-scale feedback scenarios at ~2 sigma.
Presents 24 AREPO+IllustrisTNG zoom-in simulations of clusters above 10^15 solar masses showing converged magnetic fields with volume-averaged plasma beta approximately 100 inside R200 after z~1.2, declining Faraday rotation profiles, and intermittent Braginskii heating approaching cooling rates in
SAMOS demonstrates reliable target acquisition, programmable multi-object spectroscopy at R~2500 and R~10000, and 0.3 Å calibration accuracy after on-sky commissioning at SOAR.
citing papers explorer
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Simulating megaparsec-scale jets of radio galaxies: Magneto-hydrodynamics of jets reaching 5 Mpc
3D MHD simulations show high-thrust, magnetically stabilized jets reach 5 Mpc in 15 Myr while weaker jets disrupt at ~3 Mpc over 35 Myr.
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A merger shock traced by radio arcs and ultra-long radio tails in galaxy cluster A2142
X-ray detection of M~1.3 merger shock in A2142, reproduced by off-axis merger simulations, with radio arcs interpreted as shock-induced vortex rings and ultra-long tails explained by post-shock electron re-acceleration and plasma stretching.
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Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts
FRB dispersion measures directly constrain suppression of the matter power spectrum due to feedback at k ~ 0.1-3 h/Mpc, reduce posterior variance by a factor of ~8 at k~1 h/Mpc, and exclude extreme large-scale feedback scenarios at ~2 sigma.
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The PICO-Cluster Project: presenting the galaxy cluster sample and studying magnetic field growth, Faraday rotation and Braginskii heating
Presents 24 AREPO+IllustrisTNG zoom-in simulations of clusters above 10^15 solar masses showing converged magnetic fields with volume-averaged plasma beta approximately 100 inside R200 after z~1.2, declining Faraday rotation profiles, and intermittent Braginskii heating approaching cooling rates in
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Operational capabilities and on-sky performance of SAMOS at the completion of science commissioning
SAMOS demonstrates reliable target acquisition, programmable multi-object spectroscopy at R~2500 and R~10000, and 0.3 Å calibration accuracy after on-sky commissioning at SOAR.