activity
19952009
most citedThe Luminosity Function of the Milky Way Satellites

356 citations · 1k across the 70 of their papers we have counts for

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Showing 2001 · astro-phShow all

7 papers · 2 filters

astro-ph2001

Searching for Clusters of Galaxies with SUMSS

H. J. Buttery, G. Cotter, R. W. Hunstead +1

Statistical overdensities of radio sources in the NRAO VLA Sky Survey (NVSS) catalogue have proven to be signposts to high-redshift clusters of galaxies. A similar search for overd…

astro-ph2001

On the effects of the stellar magnetic field on the structure of T Tauri accretion discs

Y. Ulchin, O. Regev, G. A. Wynn

The structure of accretion discs around magnetic T Tauri stars is numerically calculated using a particle hydrodynamical code, in which magnetic interaction is included in the fram…

astro-ph2001

The host galaxy of GRB010222: The strongest damped Lyman-alpha system known

I. Salamanca, L. Kaper, P. M. Vreeswijk +6

Analysis of the absorption lines in the afterglow spectrum of the gamma-ray burst GRB010222 indicates that its host galaxy (at a redshift of z=1.476) is the strongest damped Lyman-…

astro-ph2001

Solar coronal observations at high frequencies

A. C. Katsiyannis, M. Mathioudakis, K. J. H. Phillips +2

The Solar Eclipse Coronal Imaging System (SECIS) is a simple and extremely fast, high-resolution imaging instrument designed for studies of the solar corona. Light from the corona…

astro-ph2001

The Recurrent Nova U Scorpii - A Type Ia Supernova Progenitor

T. D. Thoroughgood, V. S. Dhillon, S. P. Littlefair +2

We derive the mass of the white dwarf in the eclipsing recurrent nova U Sco from the radial velocity semi-amplitudes of the primary and secondary stars. Our results give a high whi…

astro-ph2001

Stochastic excitation of stellar oscillations

Reza Samadi

Excitation of solar oscillations is attribued to turbulent motions in the solar convective zone. It is also currently believed that oscillations of low massive stars (M <2 Mo) - wh…