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Central Regions of AGNs Probed by the Neutral Hydrogen
Published online by Cambridge University Press: 30 March 2016
Abstract
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The physical and kinematical conditions of the gas surrounding an active galactic nucleus (AGN) offer key diagnostics for understanding the processes occurring in the inner few kpc around the nucleus. Neutral hydrogen can give important insights on these regions. Apart from probing the presence of gas in relatively settled conditions (i.e. circumnuclear disks/tori) it can also trace the presence of extreme outflows. Some examples of these phenomena are briefly presented.
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- Copyright © Astronomical Society of Pacific 2005
References
Conway, J.E.
1999 in Highly redshifted radio lines, Carilli, C.L.
et al. eds., ASP Conf. Series
156, 259
Google Scholar
Conway, J.E.
1997, in 2nd Workshop on GPS and CSS Radio Sources, Snellen,
et al.
M.N. Publ JIVE, Leiden p.198
Google Scholar
Morganti, R.
2002, in Issues in Unification of Active Galactic Nuclei, Maiolino, R.
et al. eds., ASP Conference Proceedings, Vol. 258 p.63 (astro-ph/0109056)Google Scholar
Morganti,
et al.
2003a, in Recycling Intergalactic and Interstellar Matter, IAU Symposium
217, eds. Duc, P.-A.
et al., in press (astro-ph/0310629)Google Scholar
Morganti, R., Oosterloo, T.A., Emonts, B.H.C., van der Hulst, J.M., & Tadhunter, C.N.
2003b, ApJLetter
593, L69
CrossRefGoogle Scholar
Morganti, R.
et al.
2002, 6th European VLBI Network Symposium, Ros, E.
et al. (Eds.), MPIfR, Bonn, Germany p. 171
Google Scholar
van Langevelde, H.J., Pihlstrom, Y.M., Conway, J.E., Jaffe, W., & Schilizzi, R.T.
2000, A&A
354, 45
Google Scholar
van der Marel, R.
2001, in ‘Galaxies and their Constituents at the Highest Angular Resolutions’ IAU Symp. 205, Schilizzi, R.
et al. eds., ASP, p.l54
Google Scholar
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