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

12k citations

Showing 2020 · astro-ph.SRShow all

40 papers · 2 filters

astro-ph.SR2020★ 17 cited

AU-scale radio imaging of the wind collision region in the brightest and most luminous non-thermal colliding wind binary Apep

B. Marcote, J. R. Callingham, M. De Becker +5

The recently discovered colliding-wind binary (CWB) Apep has been shown to emit luminously from radio to X-rays, with the emission driven by a binary composed of two Wolf-Rayet (WR…

astro-ph.SR2020★ 9 cited

Investigating three Sirius-like systems with SPHERE

R. Gratton, V. D'Orazi, T. A. Pacheco +61

Sirius-like systems are wide binaries composed of a white dwarf (WD) and a companion of a spectral type earlier than M0. The WD progenitor evolves in isolation, but its wind during…

astro-ph.SR2020★ 11 cited

New X-ray detections of known Wolf-Rayet stars

Yael Naze, Eric Gosset, Quentin Marechal

Using XMM-Newton, we undertook a dedicated project to search for X-ray bright wind-wind collisions in 18 WR+OB systems. We complemented these observations with Swift and Chandra da…

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.SR2020★ 58 cited

Reinvestigating Cen AB in light of asteroseismic forward and inverse methods

Sébastien Salmon, Valérie Van Grootel, Gaël Buldgen +2

The Cen stellar system is the closest neighbour to our Sun. Its main component is a binary composed of two main-sequence stars, one more massive than the Sun and one less massi…

astro-ph.SR2020★ 18 cited

Testing abundance-age relations beyond solar analogues with Kepler LEGACY stars

Thierry Morel, Orlagh L. Creevey, Josefina Montalban +2

We present abundances of 21 elements in a sample of 13 bright FG dwarfs drawn from the Kepler LEGACY sample to examine the applicability of the abundance-age relations to stars wit…