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

12k citations

Showing 2013 · astro-ph.SRShow all

58 papers · 2 filters

astro-ph.SR2013★ 9 cited

Extensive study of HD 25558, a long-period double-lined binary with two SPB components

Á. Sódor, P. De Cat, D. J. Wright +33

We carried out an extensive observational study of the Slowly Pulsating B (SPB) star, HD 25558. The ~2000 spectra obtained at different observatories, the ground-based and MOST sat…

astro-ph.SR2013★ 1 cited

The feedback of massive stars on interstellar astrochemical processes

Michael De Becker

Astrochemistry is a discipline that studies physico-chemical processes in astrophysical environments. Such environments are characterized by conditions that are substantially diffe…

astro-ph.SR2013★ 30 cited

Wind collisions in three massive stars of Cyg OB2

Constantin Cazorla, Yael Naze, Gregor Rauw

Aims: We wish to study the origin of the X-ray emission of three massive stars in the Cyg OB2 association: Cyg OB2 #5, #8A, #12. Methods: To this aim, dedicated X-ray observations…

astro-ph.SR2013★ 63 cited

Study of KIC 8561221 observed by Kepler: an early red giant showing depressed dipolar modes

R. A. Garcia, F. Perez Hernandez, O. Benomar +23

The continuous high-precision photometric observations provided by the CoRoT and Kepler space missions have allowed us to better understand the structure and dynamics of red giants…

astro-ph.SR2013★ 22 cited

A search for pulsations in the HgMn star HD 45975 with CoRoT photometry and ground-based spectroscopy

T. Morel, M. Briquet, M. Auvergne +28

The existence of pulsations in HgMn stars is still being debated. To provide the first unambiguous observational detection of pulsations in this class of chemically peculiar object…

astro-ph.SR2013★ 91 cited

Searching for companions down to 2 AU from beta Pictoris using the L'-band AGPM coronagraph on VLT/NACO

Olivier Absil, Julien Milli, Dimitri Mawet +6

Context. The orbit of the giant planet discovered around beta Pic is slightly inclined with respect to the outer parts of the debris disc, which creates a warp in the inner debris…