Pulsars, transients and relativistic astrophysics

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UYSO 1 - An extremely young massive stellar object

DENSE INTERSTELLAR MEDIUM IN GALAXIES 91 (2004) 645-648

Authors:

J Forbrich, K Schreyer, B Posselt, R Klein, T Henning
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Viscous shear instability in weakly magnetized, dilute plasmas

ASTROPHYSICAL JOURNAL 616:2 (2004) 857-864
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Exploring the Nature of Weak Chandra Sources near the Galactic Centre

(2003)

Authors:

RM Bandyopadhyay, KM Blundell, Ph Podsiadlowski, JCA Miller-Jones, QD Wang, WN Brandt, S Rappaport, E Pfahl
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Short-Term Radio-X-ray Correlations of Cygnus X-1

(2003)

Authors:

T Gleissner, J Wilms, GG Pooley, MA Nowak, K Pottschmidt, S Markoff, M Klein-Wolt, RP Fender, R Staubert
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Searching for clusters with SUMSS

Revista Mexicana de Astronomia y Astrofisica: Serie de Conferencias 17 (2003) 263

Authors:

HJ Buttery, G Cotter, RW Hunstead, EM Sadler

Abstract:

Searches for statistical overdensities of radio sources in the NRAO VLA Sky Survey (NVSS) survey have led to the detection of high redshift clusters of galaxies (Cotter et al. 2002; Croft et al. 2001). We have carried out a similar search for overdensities using the Sydney University Molonglo Sky Survey (SUMSS). Radio observations at 20/13 cm have been made of these candidates at the Australia Telescope Compact Array (ATCA) revealing sources of diffuse cluster emission as well as groups of FR1 sources showing structures associated with clusters, indicating a cluster "hit-rate" of about 70%.
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