Radio Jet-ISM Feedback on Sub-Galactic Scales

Kristina Nyland; D Mukherjee; Mark Lacy; Isabella Prandoni; J.J. Harwood; K Alatalo; Geoffrey Bicknell; Bjorn Emonts

Radio Jet-ISM Feedback on Sub-Galactic Scales

Kristina Nyland, D Mukherjee, Mark Lacy, Isabella Prandoni, J.J. Harwood, K Alatalo, Geoffrey Bicknell, Bjorn Emonts

Research output: Contribution to conference › Paper › peer-review

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.

Original language	English
Pages	457-463
Publication status	Published - 2018
Event	Science with a Next Generation Very Large Array, ASP Conference Series - Duration: 1 Jan 2018 → … http://www.aspbooks.org/a/volumes/table_of_contents/517

Conference

Conference	Science with a Next Generation Very Large Array, ASP Conference Series
Period	1/01/18 → …
Internet address	http://www.aspbooks.org/a/volumes/table_of_contents/517

Cite this

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title = "Radio Jet-ISM Feedback on Sub-Galactic Scales",

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.",

author = "Kristina Nyland and D Mukherjee and Mark Lacy and Isabella Prandoni and J.J. Harwood and K Alatalo and Geoffrey Bicknell and Bjorn Emonts",

year = "2018",

language = "English",

pages = "457--463",

note = "Science with a Next Generation Very Large Array, ASP Conference Series ; Conference date: 01-01-2018",

url = "http://www.aspbooks.org/a/volumes/table_of_contents/517",

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TY - CONF

T1 - Radio Jet-ISM Feedback on Sub-Galactic Scales

AU - Nyland, Kristina

AU - Mukherjee, D

AU - Lacy, Mark

AU - Prandoni, Isabella

AU - Harwood, J.J.

AU - Alatalo, K

AU - Bicknell, Geoffrey

AU - Emonts, Bjorn

PY - 2018

Y1 - 2018

N2 - 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.

AB - 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.

M3 - Paper

SP - 457

EP - 463

T2 - Science with a Next Generation Very Large Array, ASP Conference Series

Y2 - 1 January 2018

ER -

Radio Jet-ISM Feedback on Sub-Galactic Scales

Abstract

Conference

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