MERLIN polarimetry of the OH masers in IRAS 20406+2953     

I. Bains  A. M. S. Richards  T. M. Gledhill  J. A. Yates 《Monthly notices of the Royal Astronomical Society》2004,354(2):529-542

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A radio jet in the prototypical symbiotic star Z And?     

C. Brocksopp  J. L. Sokoloski  C. Kaiser  A. M. Richards  T. W. B. Muxlow  N. Seymour 《Monthly notices of the Royal Astronomical Society》2004,347(2):430-436

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Radial distribution and strong lensing statistics of satellite galaxies and substructure using high-resolution ΛCDM hydrodynamical simulations     

Andrea V. Macciò  Ben Moore  Joachim Stadel  Jürg Diemand 《Monthly notices of the Royal Astronomical Society》2006,366(4):1529-1538

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Morphological evolution of discs in clusters     

Chiara Mastropietro  Ben Moore  Lucio Mayer  Victor P. Debattista  Rocco Piffaretti  Joachim Stadel 《Monthly notices of the Royal Astronomical Society》2005,364(2):607-619

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Jets in the Fanaroff–Riley class I radio galaxies PKS B1234−723, MRC 1452−517 and PKS B2148−555     

Ben D.Lloyd  Paul A.Jones 《Monthly notices of the Royal Astronomical Society》2002,331(3):717-730

We present radio observations made with the Australia Telescope Compact Array to study the jets and lobes of three Fanaroff–Riley class I (FR I) radio galaxies: PKS B1234−723, 1452−517 and B2148−555. The total intensity and polarization radio images of the FR I jets are used to determine jet brightness and width variations, magnetic field structure and fractional polarization. The equipartition pressure is determined as a function of distance from the galaxies to probe the intergalactic medium.  相似文献   

Simulating H2O Maser Emission in the Mass Outflows from Evolved Stars     

J. A. Yates  E. M. L. Humphreys  A. M. S. Richards 《Astrophysics and Space Science》1997,251(1-2):285-288

The combination of a time-dependent spherically symmetric hydrodynamic model of stellar atmosphere pulsation and a radiation transport code, which incorporates maser saturation theory, enabled us to synthesise maps and spectra of H₂O maser emission from the circumstellar envelopes of long period variable stars. The synthetic maps and spectra compare favourably with observed 22, 321 and 325 GHz H₂O maser emission. As is observed in H₂O maser regions the peak emission occurs between 3–8 stellar radii from the star. The calculated H₂O maser regions are in conditions of n_H2 = 10⁶ − 10⁸ cm⁻³, assuming a fractional abundance of 10⁻⁴; kinetic temperatures of 550–3000 K; dust ensemble temperatures of 500–1200 K and an accelerating velocity field. The IR radiation field is explicitly included in the radiation transport model, incorporating the latest absorption efficiency data for silicates from Draine. We reproduce the features seen in high angular resolution MERLIN spectral line datacubes. This shows that a mass outflow model which extends the photosphere using pulsations and incorporates radiation pressure on silicate based dust particles can produce the observed data on small (10-mas) angular scales. This revised version was published online in September 2006 with corrections to the Cover Date.  相似文献   

A multi‐technique study of the glacial stratigraphy of Co. Clare and Co. Kerry,southwest Ireland     

Andrew E. Richards 《第四纪科学杂志》2002,17(3):261-276

A multi‐technique approach has been adopted in a study of the lithostratigraphy of glacial deposits in southwestern Ireland, including clast lithological analysis, fine sand geochemistry, low frequency mass specific susceptibility and fine sand calcium carbonate (equivalent) content. A revised lithostratigraphical scheme is suggested for the Quaternary glacial deposits of the region, together with a simple strategy that may be adopted for stratigraphical studies in other regions of southern Ireland. It appears that geochemical determinations via inductively coupled plasma–atomic absorption spectrometry are particularly useful in characterising and discriminating between till units within local stratigraphical studies and may be used to inform the applicability of other utilitarian techniques for use on a regional scale. Copyright © 2002 John Wiley & Sons, Ltd.  相似文献   

Deflection of plumes by mantle shear flow: experimental results and a simple theory   总被引：4，自引：0，他引：4  

Mark A. Richards  Ross W. Griffiths 《Geophysical Journal International》1988,94(3):367-376

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First results from the Very Small Array – I. Observational methods     

Robert A. Watson  Pedro Carreira  Kieran Cleary  Rod D. Davies  Richard J. Davis  Clive Dickinson  Keith Grainge †  Carlos M. Gutiérrez  Michael P. Hobson  Michael E. Jones  Rüdiger Kneissl  Anthony Lasenby  Klaus Maisinger  Guy G. Pooley  Rafael Rebolo  José Alberto Rubiño-Martin ‡  Ben Rusholme §  Richard D. E. Saunders  Richard Savage  Paul F. Scott  An&#;e Slosar  Pedro J. Sosa Molina  Angela C. Taylor  David Titterington  Elizabeth Waldram  Althea Wilkinson 《Monthly notices of the Royal Astronomical Society》2003,341(4):1057-1065

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APEX-SZ a Sunyaev–Zel’dovich galaxy cluster survey     

D. Schwan  F. Bertoldi  S. Cho  M. Dobbs  R. Guesten  N. W. Halverson  W. L. Holzapfel  E. Kreysa  T. M. Lanting  A. T. Lee  M. Lueker  J. Mehl  K. Menten  D. Muders  M. Myers  T. Plagge  A. Raccanelli  P. Schilke  P. L. Richards  H. Spieler  M. White 《New Astronomy Reviews》2003,47(11-12):933

The APEX-SZ experiment is a sky survey designed to discover galaxy clusters via the Sunyaev–Zel’dovich effect at millimeter wavelengths. We describe the components of the instrument, including the 12 m Atacama Pathfinder Experiment telescope, optics, Transition-edge sensor bolometer array and SQUID readout. APEX-SZ will begin observations in 2004.  相似文献