Exploring the Cold Universe: From Obscured Active Galactic Nuclei, Interstellar to Circumgalactic Media at z ~ 5 - 7

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• Seiji Fujimoto (Copenhagen)
• Friday 10 December 2021, 11:30-12:30
• via zoom .

If you have a question about this talk, please contact Martin Haehnelt.

The cosmic infrared background light is known to have energy comparable to the optical background light, suggesting the importance of infrared observations to understand the other aspect of the universe obscured by cold materials. In this seminar, I will present our latest research on the formation and evolution of galaxies at z_{5-7 in a wide range of scales, including active galactic nuclei ( 100 pc to 5 kpc), and circumgalactic media (CGM; ~5-20 kpc), based on the latest (sub)millimeter observations with ALMA and NOEMA. I will discuss what is taking place in the cold side of the early universe, highlighting three recent discoveries: i) CGM-scale [CII]158um gas halos, ii) differential 3D structures between neutral and ionized gases in the ISM, and iii) a young, transitioning-phase quasar forming in a dust-enshrouded starburst at z=7.2.}

This talk is part of the Galaxies Discussion Group series.

This talk is included in these lists:

• Cambridge Astronomy Talks
• Combined External Astrophysics Talks DAMTP
• Cosmology, Astrophysics and General Relativity
• Galaxies Discussion Group
• Institute of Astronomy Talk Lists
• Kavli Institute for Cosmology Talk Lists
• via zoom

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