2-6 September 2024
CJD Bonn Castell
Europe/Berlin timezone
- evn2024@mpifr.de
Support
Session II: Black hole and galaxy evolution -- Chair: Paola Castangia
Place
Location: CJD Bonn Castell
Address: Graurheindorfer Str. 149, 53117 Bonn
Date:
2 Sep 11:00 - 12:30
Description
30m Invited Talk
4x 15min Contributed Talk
Timetable | Contribution List
Displaying 5
contributions
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5
The physics that drives galaxy evolution operates on a large dynamic range of spatial scales and across a wide range of gas phases. The unique perspective enabled by high-resolution radio continuum, polarimetric, and spectral line observations offers important insights not possible in other parts of the electromagnetic spectrum. I will present several examples of this, where SKA precursors/pathfin
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Presented by Prof. Roger DEANE
on
2/9/2024
at
9:00
Radio galaxies (RGs) are active galactic nuclei (AGN) able to launch relativistic jets, the most energetic phenomena in the Universe, which can have a large impact on galaxy evolution. Current high-sensitivity and high-resolution surveys have shed new light on properties of RGs, particularly in the local Universe (z<0.3) and at low luminosities (<10^24 W/Hz a 1.4 GHz), where the bulk of the AGN po
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Presented by Dr. Ranieri D. BALDI
on
2/9/2024
at
10:00
The evolutionary stage of a powerful radio source originated by an AGN is thought to be related to its linear size. However, the fraction of young radio sources in flux density-limited samples is much larger than what is expected from the number counts of large radio sources, suggesting the existence of short-lived objects and/or intermittency of jet activity. Determining the incidence of young bu
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Presented by Dr. Monica ORIENTI
on
2/9/2024
at
10:15
The advent of new generation radio telescopes is opening new possibilities on the classification and study of extragalactic high-energy sources, specially the underrepresented ones like radio galaxies. Among these, Giant Radio Galaxies (GRG, larger than 0.7 Mpc) are among the most extreme mani- festations of the accretion/ ejection processes on supermassive black holes. Our recent studies have sho
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Presented by Dr. Gabriele BRUNI
on
2/9/2024
at
9:45
The high angular resolution and sensitivity of VLBI offers a unique tool to identify and study AGN and star-formation activity over cosmic time. VLBI observations are crucial for identifying young radio sources and unveiling older restarted radio sources. Also, radio imaging over a large range of angular scales is needed to determine the role of black hole feedback and jet-induced star formation i
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Presented by Célestin HERBÉ-GEORGE
on
2/9/2024
at
9:30