output
19922026
most citedThe SIESTA method for ab initio order-N materials simulation

12k citations

Showing 2014 · astro-ph.SRShow all

64 papers · 2 filters

astro-ph.SR2014★ 20 cited

Search for magnetic fields in particle-accelerating colliding-wind binaries

C. Neiner, J. Grunhut, B. Leroy +2

Some colliding-wind massive binaries, called particle-accelerating colliding-wind binaries (PACWB), exhibit synchrotron radio emission, which is assumed to be generated by a stella…

astro-ph.SR2014★ 70 cited

The VLTI / PIONIER near-infrared interferometric survey of southern T Tauri stars. I. First results

Fabien Anthonioz, François Ménard, Christophe Pinte +15

Context : The properties of the inner disks of bright Herbig AeBe stars have been studied with near infrared (NIR) interferometry and high resolution spectroscopy. The continuum an…

astro-ph.SR2014★ 6 cited

Magnetic fields in O-, B- and A-type stars on the main sequence

Maryline Briquet

In this review, the latest observational results on magnetic fields in main-sequence stars with radiative envelopes are summarised together with the theoretical works aimed at expl…

astro-ph.SR2014★ 35 cited

B fields in OB stars (BOB): on the detection of weak magnetic fields in the two early B-type stars beta CMa and epsilon CMa

L. Fossati, N. Castro, T. Morel +15

Within the context of the "B fields in OB stars (BOB)" collaboration, we used the HARPSpol spectropolarimeter to observe the early B-type stars beta CMa (HD44743; B1 II/III) and ep…

astro-ph.SR2014★ 61 cited

The Gaia-ESO Survey: CNO abundances in the open clusters Trumpler 20, NGC 4815, and NGC 6705

G. Tautvaišienė, A. Drazdauskas, Š. Mikolaitis +30

Aim of this work is to determine C, N, and O abundances in stars of Galactic open clusters of the Gaia-ESO survey and to compare the observed abundances with those predicted by cur…

astro-ph.SR2014★ 35 cited

Stellar acoustic radii, mean densities and ages from seismic inversion techniques

Gaël Buldgen, Daniel Roy Reese, Marc-Antoine Dupret +1

Context. Determining stellar characteristics such as the radius, the mass or the age is crucial when studying stellar evolution, exoplanetary systems or characterising stellar popu…