The cluster environment of Abell 3667

ASTR SOC P 250 (2002) 432-436

Authors:

M Johnston-Hollitt, RD Ekers, RW Hunstead

Abstract:

Abell 3667 is a rich X-ray luminous southern cluster of galaxies at a redshift of 0.055. The properties of this cluster suggest that it is probably in a post-merger state. Recent radio observations taken with the Australia Telescope Compact Array (ATCA) have allowed a detailed investigation of the environment in this cluster. We present here a synopsis of these observations.

The death of FR II radio sources and their connection with radio relics

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 336:2 (2002) 649-658

Authors:

CR Kaiser, G Cotter

The dynamical structure of nonradiative black hole accretion flows

ASTROPHYSICAL JOURNAL 573:2 (2002) 738-748

Authors:

JF Hawley, SA Balbus

The early days of a radio source

ASTR SOC P 250 (2002) 404-407

Authors:

D Dallacasa, C Stanghellini

Abstract:

We present a sample of bright compact sources with peaked radio spectra. The sample is likely to contain a mixture of a number of very young radio sources and some beamed objects whose radio emission is dominated by a single component. Flux density Variability is common among these sources, which we call "High Frequency Peakers" (HFPs).

The environments of FR II radio sources

ASTR SOC P 250 (2002) 358-362

Authors:

MJ Hardcastle, DM Worrall

Abstract:

Using ROSA T observations, we estimate gas pressures in the X-ray-emitting media surrounding 63 FR II radio galaxies and quasars. We compare these pressures with the internal pressures of the radio-emitting plasma estimated by assuming minimum energy or equipartition. The majority of the radio sources (including 12/13 sources with modelled, spatially resolved X-ray emission) Appear to be underpressured with respect to the external medium, suggesting that simple minimum-energy arguments underestimate the sources' internal energy densities. Some consequences of this result are discussed.