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A universal radio–X-ray correlation in low/hard state black hole binaries

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 344:1 (2003) 60-72

Authors:

E Gallo, RP Fender, GG Pooley
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LOFAR: A NEW RADIO TELESCOPE FOR LOW FREQUENCY RADIO OBSERVATIONS: SCIENCE AND PROJECT STATUS

World Scientific Publishing (2003) 69-76

Authors:

H RÖTTGERING, AG DE BRUYN, RP FENDER, J KUIJPERS, MP VAN HAARLEM, M JOHNSTON-HOLLITT, GK MILEY
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Status of the CLEO III silicon tracker

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment Elsevier 511:1-2 (2003) 11-15

Authors:

E von Toerne, MS Alam, JP Alexander, A Anastassov, K Arndt, A Bean, F Blanc, G Boyd, GW Brandenburg, JW Cherwinka, JE Duboscq, E Eckhart, A Ershov, J Fast, AD Foland, PI Hopman, KK Gan, Y Gao, HP Kagan, S Kane, L Kazkaz, R Kass, D Kim, J Lee, AJ Magerkurth, D Miller, J Miyamoto, M Neustadt, J Oliver, V Pavlunin, C Rush, T Selby, H Severini, M Shepherd, I Shipsey, P Skubic, T Smith, P Sterner, S Timm, D Tournear, CW Ward, M Weinberger, Q Zhang, X Zhao, MM Zoeller
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The Chemical Composition of Two Supergiants in the Dwarf Irregular Galaxy WLM

The Astronomical Journal American Astronomical Society 126:3 (2003) 1326-1345

Authors:

Kim A Venn, Eline Tolstoy, Andreas Kaufer, Evan D Skillman, Sonya M Clarkson, Stephen J Smartt, Danny J Lennon, Rolf P Kudritzki
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The absorbing haloes around high-redshift radio galaxies: the UVES view

NEW ASTRON REV 47:4-5 (2003) 279-283

Authors:

RJ Wilman, MJ Jarvis, HJA Rottgering, L Binette

Abstract:

We summarise the properties of the absorbing haloes around two high-redshift radio galaxies studied with the VLT-UVES echelle spectrograph. The absorbers in 0943 - 242 (z = 2.92) exhibit little further structure compared with previous data-the main absorber still has N(HI) similar or equal to 10(19) cm(-2)-reinforcing the picture in which the absorbing gas occupies a smooth shell beyond the emission line halo. In 0200+015 (z = 2.23) the main absorber now splits into two spatially-resolved systems with N(HI) = 4 x 10(14) cm(-2), one of which has strong CIV absorption, implying a metallicity of Z similar or equal to 10 Zcircle dot. We explain the differences between the two sources with an evolutionary scenario, invoking interaction with the expanding radio source and metal enrichment via a starburst superwind. (C) 2003 Elsevier B.V. All rights reserved.
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