activity
20032024
most citedNLTE line formation of Fe for late-type stars. I. Standard stars with 1D and <3D> model atmospheres

356 citations · 5.7k across the 76 of their papers we have counts for

collaborators

77 papers

astro-ph.IM2024

The Stagger Code for Accurate and Efficient, Radiation-Coupled MHD Simulations

Robert F. Stein, Åke Nordlund, Remo Collet +1

We describe the Stagger Code for simulations of magneto-hydrodynamic (MHD) systems. This is a modular code with a variety of physics modules that will let the user run simulations…

astro-ph.SR2023★ 18 cited

3D Stagger model atmospheres with FreeEOS I. Exploring the impact of microphysics on the Sun

Yixiao Zhou, Anish M. Amarsi, Victor Aguirre Børsen-Koch +3

Three-dimensional radiation-hydrodynamics (3D RHD) simulations of stellar surface convection provide valuable insights into many problems in solar and stellar physics. However, alm…

astro-ph.SR2021

The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines

A. M. Amarsi, N. Grevesse, M. Asplund +1

Carbon, nitrogen, and oxygen are the fourth, sixth, and third most abundant elements in the Sun. Their abundances remain hotly debated due to the so-called solar modelling problem…

astro-ph.SR2020★ 6 cited

The signature of granulation in a solar power spectrum as seen with COBOLD

Mia S. Lundkvist, Hans-Günter Ludwig, Remo Collet +1

The granulation background seen in the power spectrum of a solar-like oscillator poses a serious challenge for extracting precise and detailed information about the stellar oscilla…

astro-ph.SR2020

Sun-like Oscillations in the Population II giant HD 122563

Orlagh Creevey, Frédéric Thévenin, Frank Grundahl +8

We have been monitoring the metal-poor Population II giant, HD 122563, for radial velocity variations since 2016 using the SONG telescope on Tenerife. We have detected the global s…

astro-ph.SR2020★ 19 cited

Convective Excitation and Damping of Solar-like Oscillations

Yixiao Zhou, Martin Asplund, Remo Collet +1

The last decade has seen a rapid development in asteroseismology thanks to the CoRoT and Kepler missions. With more detailed asteroseismic observations available, it is becoming po…