HI absorption from the central kpc of radio galaxies: effect of orientation or interstellar medium?

R. Morganti; T. A. Oosterloo; C. N. Tadhunter; K. A. Wills; G. van Moorsel; A. Capetti; R. Fanti; P. Parma; H. de Ruiter

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HI absorption from the central kpc of radio galaxies: effect of orientation or interstellar medium?

R. Morganti·T. A. Oosterloo·C. N. Tadhunter·K. A. Wills·G. van Moorsel·A. Capetti·R. Fanti·P. Parma·H. de Ruiter

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Abstract

We present a summary of recent studies of HI absorption in radio galaxies. The results show how the absorption can be due to a variety of phenomena and how they can help us in understanding more of what is happening in and around AGNs.

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R. Morganti, T. A. Oosterloo, C. N. Tadhunter, K. A. Wills, G. van Moorsel, A. Capetti, R. Fanti, P. Parma, H. de Ruiter. 2001-07-26. HI absorption from the central kpc of radio galaxies: effect of orientation or interstellar medium?. https://arxiv.org/abs/astro-ph/0107501

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