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19982005
most cited21st Century VLBI: Deep Wide-Field Surveys

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astro-ph2000

HI absorption and the ISM around radio galaxies

R. Morganti, T. A. Oosterloo, C. N. Tadhunter +3

We 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…

astro-ph2000

Parsec-scale structures of radio galaxies in the 2-Jy sample

T. Venturi, R. Morganti, T. Tzioumis +1

In this paper we present the results of VLBI observations of six radio galaxies belonging to the 2-Jy sample. The selected objects are 3C17, PKS 0620-52, PKS 0625-35, PKS 1318-43,…

astro-ph2000

HI in Early-Type Galaxies

T. Oosterloo, R. Morganti, E. M. Sadler

We briefly discuss the main differences between the HI properties of luminous and low-luminosity early-type galaxies. In luminous early-type galaxies the HI is often irregularly di…

astro-ph2000

Neutral and ionized gas distribution in and around the radio galaxy Coma A

R. Morganti, T. Oosterloo, C. N. Tadhunter +1

HI absorption has been detected with the WSRT against both lobes of the radio galaxy Coma A. This radio galaxy could be expanding in a particularly gas rich environment, perhaps th…

astro-ph2000

The HST snapshot survey of the B2 sample of low luminosity radio-galaxies: a picture gallery

A. Capetti, H. R. de Ruiter, R. Fanti +3

A Hubble Space Telescope snapshot survey of the B2 sample of low luminosity radio galaxies has, at present, produced V and I images of 41 objects. Together with 16 images of B2 sou…

astro-ph2000

HI absorption in radio galaxies

R. Morganti, T. A. Oosterloo, G. van Moorsel +2

Twenty-two powerful radio galaxies have been searched for HI absorption. We find the highest probability of detecting HI in absorption among narrow-line compact (or small) galaxies…