2024-W24-5

BH

2406.09064

  • The nature of the accretion physics in quiescent black hole system LB-1

2406.08535

  • Warm Hawking Relics From Primordial Black Hole Domination

AGN

2406.08861

  • Spatially resolved analysis of Stellar Populations in NGC 2992: Impact of AGN feedback

2406.08720

  • Updated Picture of the Active Galactic Nuclei with Dusty/Dust-free Gas Structures and Effects of the Radiation Pressure

2406.08622

  • The SDSS-V Black Hole Mapper Reverberation Mapping Project: CIV BAL Acceleration in the Quasar SBS 1408+544

2406.08547

  • AGN Feedback in Quiescent Galaxies at Cosmic Noon Traced by Ionized Gas Emission

Galaxy

2406.08561

  • Theory and Observation of Winds from Star-Forming Galaxies

2406.09113

  • The Milky Way as seen by Classical Cepheids I: distances based on mid-infrared photometry

2406.09127

  • The Milky Way as Seen by Classical Cepheids II: Spiral Structure

2406.08935

  • Dense Outflowing Molecular Gas in Massive Star-forming Regions

2406.08823

  • Effects of Halo Spin on Bar Formation in Disk Galaxies

Galaxy cluster

2406.09221

  • A 100 kpc Ram Pressure Tail Trailing the Group Galaxy NGC 2276

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作者:cc
链接:https://www.techfm.club/p/130990.html
来源:TechFM
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