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19992006
most citedInvestigating grain growth in disks around southern T Tauri stars at millimetre wavelengths

100 citations · 105 across the 4 of their papers we have counts for

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astro-ph2006100 cited

Investigating grain growth in disks around southern T Tauri stars at millimetre wavelengths

Dave Lommen, Chris M. Wright, Sarah T. Maddison +7

CONTEXT - Low-mass stars form with disks in which the coagulation of grains may eventually lead to the formation of planets. It is not known when and where grain growth occurs, as…

astro-ph20044 cited

From truck to optical fibre: the coming-of-age of eVLBI

A. Szomoru, A. Biggs, M. A. Garrett +6

Spurred by the advent of disk-based recording systems and the nearly explosive increase of internet bandwidth, eVLBI (Parsley et al. 2004) has undergone a remarkable development ov…

astro-ph20041 cited

High output data rates with PCInt on the EVN MkIV data processor

H. J. van Langevelde, H. Verkouter, S. Parsley +3

The EVN MkIV data processor is being equipped with a high data output capability, called PCInt. In its next phase it will allow very high data output rates, up to 160 Mb/s. This fu…

astro-ph2003

Ionised, Atomic, and Molecular Gas around the Twin Radio Jets of NGC1052

R. C. Vermeulen, E. Ros, J. A. Zensus +3

The bright radio structure of the LINER elliptical galaxy NGC1052 is dominated by bi-symmetric jets on parsec scales. Features move outward on both sides of the core at v_{app}~0.2…

astro-ph2002

The Shroud Around the Twin Radio Jets in NGC 1052

R. C. Vermeulen, E. Ros, K. I. Kellermann +3

(Abridged) We discuss multiple VLBI continuum and spectral line observations and WSRT spectroscopy of NGC 1052. Sub-parsec scale features move outward at approximately 0.26c in bi-…

astro-ph2000

AGN and starbursts at high redshift: High resolution EVN radio observations of the Hubble Deep Field

M. A. Garrett, T. W. B. Muxlow, S. T. Garrington

We present deep, wide-field European VLBI Network (EVN) 1.6 GHz observations of the Hubble Deep Field (HDF) region with a resolution of 0.025 arcseconds. Above the 210 microJy/beam…