Gas outflows in radio galaxies

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dc.creatorMorganti, R.
dc.creatorOosterloo, T.
dc.creatorEmonts, B. H. C.
dc.creatorTadhunter, C. N.
dc.creatorHolt, J.
dc.date2003-10-22
dc.date.accessioned2026-07-07T02:10:44Z
dc.date.available2026-07-07T02:10:44Z
dc.descriptionWe present a summary of our recent results on gas outflows in radio galaxies. Fast outflows (up to 2000 km/s) have been detected both in ionized and neutral gas. The latter is particularly surprising as it shows that, despite the extremely energetic phenomena occurring near an AGN, some of the outflowing gas remains, or becomes again, neutral. These results are giving new and important insights on the physical conditions of the gaseous medium around an AGN.
dc.descriptionTo appear in the proceedings of the IAU Symposium #217, Recycling Intergalactic and Interstellar Matter, eds. P.-A. Duc, J. Braine, and E. Brinks, 6 pages. The full paper with high resolution images can be downloaded from http://www.astron.nl/~morganti/Papers/outflows.ps.gz
dc.identifierhttps://arxiv.org/abs/astro-ph/0310629
dc.identifierhttp://arxiv.org/abs/astro-ph/0310629
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6836
dc.subjectAstrophysics
dc.titleGas outflows in radio galaxies
dc.typetext

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