HI absorption and the ISM around radio galaxies

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dc.creatorMorganti, R.
dc.creatorOosterloo, T. A.
dc.creatorTadhunter, C. N.
dc.creatorWills, K. A.
dc.creatorTzioumis, A.
dc.creatorReynolds, J.
dc.date2000-10-24
dc.date.accessioned2026-07-07T01:56:11Z
dc.date.available2026-07-07T01:56:11Z
dc.descriptionWe present a study, done with the Australian LBA, of HI absorption for two compact radio galaxies (PKS 1549-79 and PKS 1814-63). In both the radio galaxies, the HI appears to give us information about the environment in which the radio sources are embedded, the effect that the ISM can have on the observed characteristics and the possible presence of interaction between the ISM and the radio plasma.
dc.descriptionTo appear in ``Proceedings of the 5th EVN Symposium'', Eds. J. Conway, A. Polatidis & R. Booth, Onsala Space Observatory, Chalmers Technical University, Gothenburg, Sweden (2000), 4 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0010482
dc.identifierhttp://arxiv.org/abs/astro-ph/0010482
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1908
dc.subjectAstrophysics
dc.titleHI absorption and the ISM around radio galaxies
dc.typetext

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