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2024-W08-1
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AGN

2402.10414

  • The weakness of soft X-ray intensity: possible physical reason for weak line quasars

2402.10444

  • Quasar winds caught on acceleration and deceleration

2402.10581

  • Quasar Outflow Deceleration or Acceleration: Predictions and a Search

BH

2402.10371

  • First Year of Stellar-Mass Black Hole Observations with the Imaging X-ray Polarimetry Explorer

2402.10740

  • Black-Hole-to-Halo Mass Relation From UNIOnS Weak Lensing

disk wind

2402.10315

  • A variable ionized disk wind in MAXI J1803-298 revealed by NICER

Galaxy

2402.10270

  • CLusters in the Uv as EngineS (CLUES). II. Sub-kpc scale outflows driven by stellar feedback

2402.10415

  • GTC Spectroscopic Surveys of Planetary Nebulae in the Milky Way and M31

2402.10709

  • A Multi-Resolution Method for Modelling Galaxy and Massive Black Hole Mergers

2402.10590

  • Investigating black hole accretion disks as potential polluter sources for the formation of enriched stars in globular clusters
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