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20022009
most citedThe Kernel Polynomial Method

1.1k citations

Showing 2006 · astro-phShow all

25 papers · 2 filters

astro-ph2006102 cited

Revision of VLT/UVES constraints on a varying fine-structure constant

Michael T. Murphy, John K. Webb, Victor V. Flambaum

We critically review the current null results on a varying fine-structure constant, alpha, derived from VLT/UVES quasar absorption spectra, focusing primarily on the many-multiplet…

astro-ph200633 cited

The Metallicity of Stars with Close Companions

Daniel Grether, Charles H. Lineweaver

We examine the relationship between the frequency of close companions (stellar and planetary companions with orbital periods < 5 years) and the metallicity of their Sun-like (~ FGK…

astro-ph2006114 cited

Binarity as a key factor in protoplanetary disk evolution: Spitzer disk census of the eta Chamaeleontis cluster

J. Bouwman, W. A. Lawson, C. Dominik +4

The formation of planets is directly linked to the evolution of the circumstellar (CS) disk from which they are born. The dissipation timescales of CS disks are, therefore, of dire…

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-ph200615 cited

Asteroseismology with the WIRE satellite. I. Combining Ground- and Space-based Photometry of the Delta Scuti Star Epsilon Cephei

H. Bruntt, J. C. Suarez, T. R. Bedding +10

We have analysed ground-based multi-colour Stromgren photometry and single-filter photometry from the star tracker on the WIRE satellite of the delta scuti star Epsilon Cephei. The…

astro-ph200650 cited

Probing variations in fundamental constants with radio and optical quasar absorption-line observations

P. Tzanavaris, M. T. Murphy, J. K. Webb +2

Nine quasar absorption spectra at 21-cm and UV rest-wavelengths are used to estimate possible variations in x=alpha^2 g_p mu, (alpha is the fine structure constant, g_p the proton…