NUGA: the IRAM survey of AGN spiral hosts

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dc.creatorGarcia-Burillo, S.
dc.creatorCombes, F.
dc.creatorEckart, A.
dc.creatorTacconi, L. J.
dc.creatorHunt, L. K.
dc.creatorLeon, S.
dc.creatorBaker, A. J.
dc.creatorEnglmaier, P. P.
dc.creatorBoone, F.
dc.creatorSchinnerer, E.
dc.creatorNeri, R.
dc.date2002-12-19
dc.date.accessioned2026-07-07T02:06:57Z
dc.date.available2026-07-07T02:06:57Z
dc.descriptionThe NUclei of GAlaxies (NUGA) project is a combined effort to carry out a high-resolution (<1'') interferometer CO survey of a sample of 12 nearby AGN spiral hosts, using the IRAM array. We map the distribution and dynamics of molecular gas in the inner 1 kpc of the nuclei with resolutions of 10-50 pc, and study the mechanisms for gas fueling of the different low-luminosity AGN. First results show evidence for the occurrence of strong m=1 gas instabilities in Seyferts. NUGA maps allow us to address the origin/nature of m=1 modes and their link with m=2 modes and acoustic instabilities, present in other targets.
dc.description1 gzipped tar file containing 1 Latex file + 3 eps figures. Proceedings of ''Active Galactic Nuclei: from Central Engine to Host Galaxy'', meeting held in Meudon, France, July 23-27, 2002, Eds.: S. Collin, F. Combes and I. Shlosman. To be published in ASP Conference Series
dc.identifierhttps://arxiv.org/abs/astro-ph/0212451
dc.identifierhttp://arxiv.org/abs/astro-ph/0212451
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5541
dc.subjectAstrophysics
dc.titleNUGA: the IRAM survey of AGN spiral hosts
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