Continuum EVN and MERLIN observations of Ultra Luminous Infrared Galaxies

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dc.creatorPolatidis, A. G.
dc.creatorConway, J. E.
dc.date2005-01-03
dc.date.accessioned2026-07-07T02:16:36Z
dc.date.available2026-07-07T02:16:36Z
dc.descriptionRadio imaging of ULIR galaxies is ideal to explore the connection between the starburst and the AGN phenomenon since it is unaffected by dust obscuration, and provides the required high angular resolution to distinguish between an AGN and starburst emission. We have made combined 18cm radio continuum, EVN and MERLIN observations of 13 ULIRGs that have the parsec and deci-parsec scale resolution necessary to distinguish between an AGN and supernovae remnants at the centres of these galaxies, and assess the contribution of each to the total energy distribution. Images of four galaxies are presented here.
dc.description4 pages. 8 figures. Proceedings of the 7th European VLBI Network Symposium held in Toledo, Spain on October 12-15, 2004. Editors: R. Bachiller, F. Colomer, J.-F. Desmurs, P. de Vicente (Observatorio Astronomico Nacional), p. 231-235. Needs evn2004.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0501017
dc.identifierhttp://arxiv.org/abs/astro-ph/0501017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8847
dc.subjectAstrophysics
dc.titleContinuum EVN and MERLIN observations of Ultra Luminous Infrared Galaxies
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