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

12k citations

Showing 2012 · astro-ph.SRShow all

46 papers · 2 filters

astro-ph.SR2012★ 48 cited

Mode visibilities in rapidly rotating stars

D. R. Reese, V. Prat, C. Barban +2

Context: Mode identification is a crucial step to comparing observed frequencies with theoretical ones, but has proven to be difficult in rapidly rotating stars. Aims: To further c…

astro-ph.SR2012★ 25 cited

The 2.35 year itch of Cyg OB2 #9. II. Radio monitoring

R. Blomme, Y. Naze, D. Volpi +5

Cyg OB2 #9 is one of a small set of non-thermal radio emitting massive O-star binaries. The non-thermal radiation is due to synchrotron emission in the colliding-wind region. Cyg O…

astro-ph.SR2012★ 18 cited

High-precision CoRoT space photometry and fundamental parameter determination of the B2.5V star HD 48977

Anne Thoul, Pieter Degroote, Claude Catala +10

We present the CoRoT light curve of the bright B2.5V star HD 48977 observed during a short run of the mission in 2008, as well as a high-resolution spectrum gathered with the HERME…

astro-ph.SR2012★ 216 cited

The standard flare model in three dimensions. II. Upper limit on solar flare energy

G. Aulanier, P. Demoulin, C. J. Schrijver +3

Solar flares strongly affect the Sun's atmosphere as well as the Earth's environment. Quantifying the maximum possible energy of solar flares of the present-day Sun, if any, is thu…

astro-ph.SR2012★ 57 cited

A detailed X-ray investigation of zeta Puppis - The variability on short and long timescales

Yael Naze, Lidia M. Oskinova, Eric Gosset

Stellar winds are a crucial component of massive stars, but their exact properties still remain uncertain. To shed some light on this subject, we have analyzed an exceptional set o…

astro-ph.SR2012★ 53 cited

An interferometric study of the Fomalhaut inner debris disk II. Keck Nuller mid-infrared observations

B. Mennesson, O. Absil, J. Lebreton +7

We report on high contrast mid-infrared observations of Fomalhaut obtained with the Keck Interferometer Nuller (KIN) showing a small resolved excess over the level expected from th…