activity
19942026
most cited3D non-LTE iron abundances in FG-type dwarfs

52 citations · 75 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026★ 5 cited

Magnesium isotope ratios in Milky Way and dwarf galaxy stars

M. McKenzie, S. Monty, D. Yong +8

Under the assumption of hierarchical galaxy formation, dwarf galaxies are the closest existing analogues to the high-redshift protogalaxies that merged to form the Milky Way. These…

astro-ph.SR2025★ 6 cited

The peculiar composition of the Sun is not related to giant planets

M. Carlos, A. M. Amarsi, P. E. Nissen +1

Highly-differential spectroscopic studies have revealed that the Sun is deficient in refractory elements relative to solar twins. To investigate the role of giant planets on this s…

astro-ph.SR2024★ 11 cited

A distinct halo population revealed from 3D non-LTE magnesium abundances

T. Matsuno, A. M. Amarsi, M. Carlos +1

Magnesium is one of the important elements in stellar physics as an electron donor and in Galactic Archaeology as a discriminator of different stellar populations. However, previou…

astro-ph.GA2023

Abundances of iron-peak elements in accreted and in situ born Galactic halo stars

P. E. Nissen, A. M. Amarsi, Á. Skúladóttir +1

Previous work on the abundances of C, O, Na, Mg, Si, Ca, Ti, Cr, Mn, Fe, Ni, Cu, and Zn in low-alpha (accreted) and high-alpha (in situ born) halo stars is extended to include the…

astro-ph.SR2022★ 52 cited

3D non-LTE iron abundances in FG-type dwarfs

A. M. Amarsi, S. Liljegren, P. E. Nissen

Spectroscopic measurements of iron abundances are prone to systematic modelling errors. We present 3D non-LTE calculations across 32 STAGGER-grid models with effective temperatures…

astro-ph1994★ 1 cited

Boron in the Extreme Pop II Star HD 140283 and the Production of Light Elements in the Early Galaxy

B. Edvardsson, B. Gustafsson, S. G. Johansson +4

Using observations of the 2496.7 A B I line with the HST GHRS at a nominal resolution of 90,000, we have found the abundance of boron of HD 140283 to be log epsilon_B (= 12 + log (…