Radio Jet-ISM Feedback on Sub-Galactic Scales
Date Issued
2018
Author(s)
Nyland, K.
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Lacy, M.
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Harwood, J. J.
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Alatalo, K.
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Bicknell, G.
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Emonts, B.
Abstract
Energetic feedback by active galactic nuclei (AGNs) plays an important evolutionary role in the regulation of star formation (SF) on galactic scales. However, the effects of this feedback as a function of redshift and galaxy properties such as mass, environment, and cold gas content remain poorly understood. Given its unique combination of frequency range, angular resolution, and sensitivity, the ngVLA will serve as a transformational new tool in our understanding of how radio jets affect their surroundings. By combining broadband continuum data with measurements of the cold gas content and kinematics, the ngVLA will quantify the energetic impact of radio jets hosted by gas-rich galaxies as the jets interact with the star-forming gas reservoirs of their hosts.
Coverage
Science with a Next Generation Very Large Array
All editors
Murphy, E. J. and the ngVLA Science Advisory Council
Volume
517
Start page
457
Conferenece
Science with a Next Generation Very Large Array
Issn Identifier
1050-3390
Ads BibCode
2018ASPC..517..457N
Rights
open.access
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