Science with an ngVLA: Radio Jet-ISM Feedback on Sub-galactic Scales

Kristina Nyland; Dipanjan Mukherjee; Mark Lacy; Isabella Prandoni; Jeremy J. Harwood; Katherine Alatalo; Geoffrey Bicknell; Bjorn Emonts

Science with an ngVLA: Radio Jet-ISM Feedback on Sub-galactic Scales

Kristina Nyland, Dipanjan Mukherjee, Mark Lacy, Isabella Prandoni, Jeremy J. Harwood, Katherine Alatalo, Geoffrey Bicknell, Bjorn Emonts

Centre for Astrophysics Research (CAR)

Research output: Contribution to journal › Article › peer-review

20 Downloads (Pure)

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 (from-to)	1-9
Number of pages	9
Journal	ArXiv
Publication status	Published - 15 Oct 2018

Keywords

astro-ph.GA

Cite this

@article{0067c62797604a5fad977f6086bc6371,

title = "Science with an ngVLA: 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. ",

keywords = "astro-ph.GA",

author = "Kristina Nyland and Dipanjan Mukherjee and Mark Lacy and Isabella Prandoni and Harwood, {Jeremy J.} and Katherine Alatalo and Geoffrey Bicknell and Bjorn Emonts",

year = "2018",

month = oct,

day = "15",

language = "English",

pages = "1--9",

journal = "ArXiv",

issn = "2331-8422",

publisher = "Cornell University",

}

TY - JOUR

T1 - Science with an ngVLA: Radio Jet-ISM Feedback on Sub-galactic Scales

AU - Nyland, Kristina

AU - Mukherjee, Dipanjan

AU - Lacy, Mark

AU - Prandoni, Isabella

AU - Harwood, Jeremy J.

AU - Alatalo, Katherine

AU - Bicknell, Geoffrey

AU - Emonts, Bjorn

PY - 2018/10/15

Y1 - 2018/10/15

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.

KW - astro-ph.GA

M3 - Article

SN - 2331-8422

SP - 1

EP - 9

JO - ArXiv

JF - ArXiv

ER -

Science with an ngVLA: Radio Jet-ISM Feedback on Sub-galactic Scales

Abstract

Keywords

Fingerprint

Cite this