activity
20082016
most citedA dynamically-packed planetary system around GJ667C with three super-Earths in its habitable zone

384 citations · 566 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2016

Spectroscopic characterisation of CARMENES target candidates from FEROS, CAFE and HRS high-resolution spectra

V. M. Passegger, A. Reiners, S. V. Jeffers +9

CARMENES (Calar Alto high-Resolution search for M dwarfs with Exoearths with Near-infrared and optical Echelle Spectrographs) started a new planet survey on M-dwarfs in January thi…

astro-ph.SR2010

Magnetic fields in M-dwarfs: quantitative results from detailed spectral synthesis in FeH lines

D. Shulyak, A. Reiners, S. Wende +3

Strong surface magnetic fields are ubiquitously found in M-dwarfs with mean intensities on the order of few thousand Gauss-three orders of magnitude higher than the mean surface ma…

astro-ph.SR2010

Investigation of magnetically sensitive FeH lines

Sebastian Wende, Ansgar Reiners, Andreas Seifahrt +2

M-type stars exhibit strong magnetic fields towards decreasing effective temperatures. The measurement of these fields is complicated due to missing indicators. Molecular FeH lines…

astro-ph.SR2010★ 43 cited

Modelling the molecular Zeeman effect in M-dwarfs: methods and first results

D. Shulyak, A. Reiners, S. Wende +3

We present first quantitative results of the surface magnetic field measurements in selected M-dwarfs based on detailed spectra synthesis conducted simultaneously in atomic and mol…

astro-ph.SR2010★ 101 cited

CRIRES spectroscopy and empirical line-by-line identification of FeH molecular absorption in an M dwarf

S. Wende, A. Reiners, A. Seifahrt +1

Molecular FeH provides a large number of sharp and isolated absorption lines that can be used to measure radial velocity, rotation, or magnetic field strength with high accuracy. O…

astro-ph.SR2009★ 38 cited

3D simulations of M star atmosphere velocities and their influence on molecular FeH lines

S. Wende, A. Reiners, H. -G. Ludwig

We present an investigation of the velocity fields in early to late M-type star hydrodynamic models, and we simulate their influence on FeH molecular line shapes. The M star model…