2024-W42-2

TDE

2410.09720

  • Recurring tidal disruption events a decade apart in IRAS F01004-2237

AGN

2410.09450

  • The effects of super-Eddington accretion and feedback on the growth of early supermassive black holes and galaxies

2410.09262

  • Unveiling the quasar main sequence: illuminating the complexity of active galactic nuclei and their evolution

2410.10675

  • Hidden Cooling Flows IV: More Details on Centaurus and the Efficiency of AGN Feedback in Clusters

2410.10396

  • Persistent GeV counterpart to the microquasar GRS 1915+105

2410.10294

  • Ten years of searching for relics of AGN jet feedback through RAD@home citizen science

2410.10100

  • Could the inter-band lag of active galactic nucleus vary randomly?

BH

2410.10111

  • Constraints on primordial black holes from N_{/text{eff}} : scalar induced gravitational waves as an extra radiation component

Galaxy

2410.09705

  • The formation and survival of the Milky Way's oldest stellar disk

2410.10015

  • New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature

2410.09971

  • An acceleration-radiation model for nonthermal flares from Sgr A^/star

2410.09782

  • Revisiting the Galactic Winds in M82 II: Development of Multiphase Outflows in Simulations

2410.09205

  • From UV-bright Galaxies to Early Disks: the Importance of Turbulent Star Formation in the Early Universe

2410.09753

  • Partially Ionized Gas at Equilibrium Powered by Ultraviolet Irradiation

2410.09256

  • Measuring Star Formation Histories from Asymptotic Giant Branch Stars: A Demonstration in M31

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作者:cc
链接:https://www.techfm.club/p/161293.html
来源:TechFM
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