activity
19972012
most citedAccurate fundamental parameters for 23 bright solar-type stars

231 citations · 1.4k across the 31 of their papers we have counts for

collaborators

31 papers

astro-ph.SR2012★ 51 cited

Magnetic fields of HgMn stars

S. Hubrig, J. F. Gonzalez, I. Ilyin +8

The frequent presence of weak magnetic fields on the surface of spotted late-B stars with HgMn peculiarity in binary systems has been controversial during the two last decades. We…

astro-ph.SR2011★ 10 cited

Spectroscopic variability and magnetic fields of HgMn stars

S. Hubrig, J. F. Gonzalez, I. Ilyin +7

The discovery of exotic abundances, chemical inhomogeneities, and weak magnetic fields on the surface of late B-type primaries in spectroscopic binaries has important implications…

astro-ph.SR2011★ 13 cited

Bisectors of the HARPS Cross-Correlation-Function. The dependence on stellar atmospheric parameters

O. Basturk, T. H. Dall, R. Collet +2

Bisectors of the HARPS cross-correlation function (CCF) can discern between planetary radial-velocity (RV) signals and spurious RV signals from stellar magnetic activity variations…

astro-ph.SR2011★ 5 cited

Visualization and spectral synthesis of rotationally distorted stars

T. H. Dall, L. Sbordone

Simple spherical, non-rotating stellar models are inadequate when describing real stars in the limit of very fast rotation: Both the observable spectrum and the geometrical shape o…

astro-ph.SR2010

Oscillations and magnetic fields in the G8 star EK Eridani

T. H. Dall, M. Cunha, K. G. Strassmeier +2

Asteroseismology can provide information that is otherwise not easily accessible, like the stellar mass and the evolutionary stage. Strong magnetic fields are usually accompanied b…

astro-ph.SR2010★ 16 cited

Solar-like oscillations and magnetic activity of the slow rotator EK Eri

T. H. Dall, H. Bruntt, D. Stello +1

We aim to understand the interplay between non-radial oscillations and stellar magnetic activity and test the feasibility of doing asteroseismology of magnetically active stars. We…