Fast neutral outflows in nearby radio galaxies: a major source of feedback

Simple item page
dc.creatorMorganti, Raffaella
dc.creatorTadhunter, Clive
dc.creatorOosterloo, Tom
dc.creatorHolt, Joanna
dc.creatorEmonts, Bjorn
dc.date2007-01-15
dc.date.accessioned2026-07-07T07:41:10Z
dc.date.available2026-07-07T07:41:10Z
dc.descriptionFast (~1000 km/s) outflows of neutral gas (from 21-cm HI absorption) are detected in strong radio sources. The outflows occur, at least in some cases, at distances from the radio core that range between few hundred parsecs and kpc. These HI outflows likely originate from the interaction between radio jets and the dense surrounding medium. The estimated mass outflow rates are comparable to those of moderate starburst-driven superwinds. The impact on the evolution of the host galaxies is discussed.
dc.description4 pages, 2 figures. Conference proceedings to appear in "The Central Engine of Active Galactic Nuclei", ed. L. C. Ho and J.-M. Wang (San Francisco: ASP)
dc.identifierhttps://arxiv.org/abs/astro-ph/0701440
dc.identifierhttp://arxiv.org/abs/astro-ph/0701440
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/122004
dc.subjectAstrophysics
dc.titleFast neutral outflows in nearby radio galaxies: a major source of feedback
dc.typetext

Files

Collections

arXiv