activity
20062008
most citedHomogeneous studies of transiting extrasolar planets. I. Light curve analyses

371 citations · 1.3k across the 22 of their papers we have counts for

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Showing 2006Show all

8 papers · 1 filter

astro-ph200690 cited

A brown dwarf mass donor in an accreting binary

S. P. Littlefair, V. S. Dhillon, T. R. Marsh +3

A long standing and unverified prediction of binary star evolution theory is the existence of a population of white dwarfs accreting from sub-stellar donor stars. Such systems ough…

astro-ph200610 cited

Eclipsing Binaries in Open Clusters

John Southworth

Detached eclipsing binaries are very useful objects for calibrating theoretical stellar models and checking their predictions. Detached eclipsing binaries in open clusters are part…

astro-ph2006

Testing convection in stellar models using detached eclipsing binaries

John Southworth, Hans Bruntt

The fundamental properties of detached eclipsing binary stars can be measured very accurately, which could make them important objects for constraining the treatment of convection…

astro-ph20068 cited

Eclipsing Binary Stars from Space

H. Bruntt, J. Southworth

We have begun a programme to obtain high-precision photometry of bright detached eclipsing binary (dEB) stars with the Wide field InfraRed Explorer (WIRE) satellite. Due to the sma…

astro-ph200664 cited

Absolute dimensions of eclipsing binaries. XXIV. The Be star system DW Carinae, a member of the open cluster Collinder 228

John Southworth, J. V. Clausen

DW Carinae is a close but detached early B-type eclipsing binary in the young open cluster Cr 228. We have measured accurate physical properties of its components (masses and radii…

astro-ph200659 cited

VLT/FORS spectroscopy of faint cataclysmic variables discovered by the Sloan Digital Sky Survey

John Southworth, B. T. Gaensicke, T. R. Marsh +5

We present medium-resolution VLT/FORS2 spectroscopy of six cataclysmic variables discovered by the Sloan Digital Sky Survey. We determine orbital periods for SDSS J023322.61+005059…