2022-W52-3

BH

2212.06622

  • Possible discrimination of black hole origins from the lensing rate of DECIGO and B-DECIGO sources

AGN

S2212.06399

  • NOEMA Detection of Circumnuclear Molecular Gas in X-ray Weak Dual Active Galactic Nuclei: No Evidence for Heavy Obscuration

2212.06363

  • In-situ star formation in accretion disk and explanation for correlation between black hole mass and metallicity in AGNs

2212.06199

  • AGN cool feedback and analogy with X-ray binaries: from radiation pressure to cosmic ray driven outflows

2212.06183

  • Systematic Broad-band X-ray Study of super-Eddington Accretion onto Supermassive Black Holes. I. X-ray Continuum

2212.06179

  • Evidence of under-developed torus and broad-line region of weak emission line quasars based on their spectral energy distribution

feedback

2212.06469

  • Cosmic rays as a feedback agent in primordial galactic ecosystems

熟悉的源

2212.06585

  • Diffusion of cosmic-ray electrons in M 51 observed with LOFAR at 54 MHz

JWST

2212.06683

  • UV Luminosity Density Results at z>8 from the First JWST/NIRCam Fields: Limitations of Early Data Sets and the Need for Spectroscopy

2212.06666

  • A High Density of Bright Galaxies at z\approx10 in the A2744 region

2212.06575

  • Cosmological Model Tests with JWST

2212.06434

  • PHANGS--JWST First Results: ISM structure on the turbulent Jeans scale in four disk galaxies observed by JWST and ALMA
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