Confirmation of 77 new heavily reddened quasars at 1.5 < z < 3.9 with high luminosities and extinctions, showing they are deficient in hot and warm dust relative to blue quasars and supporting a blow-out feedback phase.
year = 1995, month = sep, volume =
6 Pith papers cite this work, alongside 350 external citations. Polarity classification is still indexing.
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astro-ph.GA 6representative citing papers
Resolved stellar-population maps of three cooling-core BCGs reveal extended young stellar populations, with a blueshifted young-star clump in A1835 interpreted as stars falling back from an AGN-driven outflow.
All three major cosmological simulations fail to reproduce the observed dependence of radio AGN fraction on galaxy mass and star formation rate.
Magnetized thermal instability can produce cold gas in galaxy cluster atmospheres at cooling-to-freefall time ratios up to about 20, matching the observed threshold range 10-30.
Simulations show jets of 10^40 erg/s and below are stalled and bent by a turbulent ISM, with a breakout threshold set by ISM ram pressure that scales as M^3 and rho_jet^-1/2.
Composite cluster stellar mass functions show marginal M* evolution at high z and a factor of 2.5 growth in stellar mass fraction from z=0.8 to 0.2 after accounting for halo mass growth.
citing papers explorer
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Star Formation Histories and Stellar Dynamics in the Central Galaxies of RX J0820.9+0752, A1835, and PKS 0745-191
Resolved stellar-population maps of three cooling-core BCGs reveal extended young stellar populations, with a blueshifted young-star clump in A1835 interpreted as stars falling back from an AGN-driven outflow.
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AGN Feedback Models and AGN Demographics I: Radio-Mode AGN in EAGLE, SIMBA and TNG100 are Inconsistent with Observations
All three major cosmological simulations fail to reproduce the observed dependence of radio AGN fraction on galaxy mass and star formation rate.
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Precipitation plausible: magnetized thermal instability in the intracluster medium
Magnetized thermal instability can produce cold gas in galaxy cluster atmospheres at cooling-to-freefall time ratios up to about 20, matching the observed threshold range 10-30.
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You Shall Not Pass! The propagation of low/moderate powered jets through a turbulent interstellar medium
Simulations show jets of 10^40 erg/s and below are stalled and bent by a turbulent ISM, with a breakout threshold set by ISM ram pressure that scales as M^3 and rho_jet^-1/2.
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The Atacama Cosmology Telescope: stellar mass growth in massive galaxy clusters from DR5 over the past 7 billion years
Composite cluster stellar mass functions show marginal M* evolution at high z and a factor of 2.5 growth in stellar mass fraction from z=0.8 to 0.2 after accounting for halo mass growth.