2024-W08-1
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
共有 0 条评论