activity
19982023
most citedSimulations of stellar convection with CO5BOLD

405 citations · 2.2k across the 54 of their papers we have counts for

collaborators

54 papers

astro-ph.SR2023★ 7 cited

VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic Pole

K. G. Strassmeier, M. Weber, D. Gruner +13

We embarked on a high-resolution optical spectroscopic survey of bright Transiting Exoplanet Survey Satellite (TESS) stars around the Northern Ecliptic Pole (NEP), dubbed the Vatic…

astro-ph.SR2022★ 7 cited

The solar photospheric silicon abundance according to CO5BOLD: Investigating line broadening, magnetic fields, and model effects

S. A. Deshmukh, H. -G. Ludwig, A. Kučinskas +5

In this work, we present a photospheric solar silicon abundance derived using CO5BOLD model atmospheres and the LINFOR3D spectral synthesis code. Previous works have differed in th…

astro-ph.SR2022★ 2 cited

On the lithium abundance of the visual binary components Boo A (G8V) and Boo B (K5V)

Klaus G. Strassmeier, Matthias Steffen

A spectroscopic investigation of the lithium resonance doublet in Boo A and Boo B in terms of both abundance and isotopic ratio is presented. We obtained new =130\,000 s…

astro-ph.SR2021

Barium lines in high-quality spectra of two metal-poor giants in the Galactic halo

G. Cescutti, C. Morossi, M. Franchini +9

Context. Theoretical results showed the possibility that neutron capture elements were produced in the early Universe by two different sources: a frequent s-process source hosted b…

astro-ph.SR2020★ 43 cited

3D spectroscopic analysis of helium-line white dwarfs

Elena Cukanovaite, Pier-Emmanuel Tremblay, Pierre Bergeron +3

In this paper, we present corrections to the spectroscopic parameters of DB and DBA white dwarfs with -10.0 < log(H/He) < -2.0, 7.5 < log(g) < 9.0 and 12000 K < T_eff < 34000 K, ba…

astro-ph.EP2020★ 10 cited

Probing the atmosphere of HD189733b with the Na I and K I lines

E. Keles, D. Kitzmann, M. Mallonn +12

High spectral resolution transmission spectroscopy is a powerful tool to characterize exoplanet atmospheres. Especially for hot Jupiters, this technique is highly relevant, due to…