Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/27615
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Nyland, K. | en_US |
dc.contributor.author | Mukherjee, D. | en_US |
dc.contributor.author | Lacy, M. | en_US |
dc.contributor.author | PRANDONI, ISABELLA | en_US |
dc.contributor.author | Harwood, J. J. | en_US |
dc.contributor.author | Alatalo, K. | en_US |
dc.contributor.author | Bicknell, G. | en_US |
dc.contributor.author | Emonts, B. | en_US |
dc.date.accessioned | 2020-10-06T07:45:30Z | - |
dc.date.available | 2020-10-06T07:45:30Z | - |
dc.date.issued | 2018 | en_US |
dc.identifier.isbn | 978-1-58381-919-7 | en_US |
dc.identifier.issn | 1050-3390 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/27615 | - |
dc.description.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. | en_US |
dc.language.iso | eng | en_US |
dc.title | Radio Jet-ISM Feedback on Sub-Galactic Scales | en_US |
dc.type | Conference paper | - |
dc.identifier.url | http://aspbooks.org/custom/publications/paper/517-0457.html | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 517 | en_US |
dc.relation.firstpage | 457 | en_US |
dc.type.referee | REF_4 | en_US |
dc.description.numberofauthors | 8 | en_US |
dc.description.international | sì | en_US |
dc.relation.alleditors | Murphy, E. J. and the ngVLA Science Advisory Council | en_US |
dc.relation.ispartofbook | Science with a Next Generation Very Large Array | en_US |
dc.relation.conferencename | Science with a Next Generation Very Large Array | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.type.miur | 273 Contributo in Atti di convegno | - |
dc.relation.series | ASTRONOMICAL SOCIETY OF THE PACIFIC CONFERENCE SERIES | en_US |
dc.identifier.adsbibcode | 2018ASPC..517..457N | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE7 Systems and Communication Engineering: Electronic, communication, optical and systems engineering | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Conference paper | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | IRA Bologna | - |
crisitem.author.orcid | 0000-0001-9680-7092 | - |
crisitem.journal.journalissn | 1050-3390 | - |
crisitem.journal.ance | E210915 | - |
Appears in Collections: | 3.01 Contributi in Atti di convegno |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
Chapter_Nyland.pdf | Pdf editoriale | 1.6 MB | Adobe PDF | View/Open |
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