output
20032009
most citedA new code for automatic determination of equivalent widths: Automatic Routine for line Equivalent widths in stellar Spectra (ARES)

328 citations

Showing 2006Show all

9 papers · 1 filter

astro-ph2006

Remarks on Statistical Properties of the Turbulent Interstellar Medium

M. A. de Avillez, D. Breitschwerdt

The supernova-driven interstellar medium in star-forming galaxies has Reynolds numbers of the order of or even larger. We study, by means of adaptive mesh refinement hydro…

astro-ph2006

Dynamical Evolution of a Supernova Driven Turbulent Interstellar Medium

Dieter Breitschwerdt, Miguel A. de Avillez

It is shown that a number of key observations of the Galactic ISM can be understood, if it is treated as a highly compressible and turbulent medium energized predominantly by super…

astro-ph200640 cited

The `666' collaboration on OGLE transits: I. Accurate radius of the planets OGLE-TR-10b and OGLE-TR-56b with VLT deconvolution photometry

Frederic Pont, Claire Moutou, Michael Gillon +14

Transiting planets are essential to study the structure and evolution of extra-solar planets. For that purpose, it is important to measure precisely the radius of these planets. He…

astro-ph200654 cited

On the Age of Stars Harboring Transiting Planets

C. Melo, N. C. Santos, F. Pont +5

Results of photometric surveys have brought to light the existence of a population of giant planets orbiting their host stars even closer than the hot Jupiters (HJ), with orbital p…

astro-ph200654 cited

Kinematics of planet-host stars and their relation with dynamical streams in the solar neighbourhood

A. Ecuvillon, G. Israelian, F. Pont +2

We present a detailed study on the kinematics of metal-rich stars with and without planets, and their relation with the Hyades, Sirius and Hercules dynamical streams in the solar n…

astro-ph2006123 cited

The HARPS search for southern extra-solar planets. IX. mu Ara, a system with four planets

F. Pepe, A. C. M. Correia, M. Mayor +13

The mu Ara planetary system is rather complex: It contains two already known planets, mu Ara b with P=640 days and mu Ara c with P=9.64 days, and a third companion on a wide but st…