activity
20152021
most citedNon-LTE analysis of K I in late-type stars

65 citations · 197 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2021★ 20 cited

Non-detection of Li in Spite plateau stars with ESPRESSO

E. X. Wang, T. Nordlander, M. Asplund +3

The detection of Li in Spite plateau stars contradicts the standard Big Bang nucleosynthesis prediction, known as the second cosmological lithium problem. We measure the isotop…

astro-ph.SR2021★ 13 cited

The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations

Yixiao Zhou, Thomas Nordlander, Luca Casagrande +5

We establish a quantitative relationship between photometric and spectroscopic detections of solar-like oscillations using ab initio, three-dimensional (3D), hydrodynamical numeric…

astro-ph.SR2019★ 65 cited

Non-LTE analysis of K I in late-type stars

Henrique Reggiani, Anish M. Amarsi, Karin Lind +7

Older GCE models predict [K/Fe] ratios as much as 1 dex lower than those inferred from stellar observations. Abundances of potassium are mainly based on analyses of the 7698 re…

astro-ph.SR2018★ 20 cited

Evidences of extragalactic origin and planet engulfment in the metal-poor twin pair HD 134439/HD 134440

Henrique Reggiani, Jorge Meléndez

Recent studies of chemical abundances in metal-poor Halo stars show the existence of different populations, which is important for studies of Galaxy formation and evolution. Here w…

astro-ph.SR2017★ 60 cited

Constraining cosmic scatter in the Galactic halo through a differential analysis of metal-poor stars

Henrique Reggiani, Jorge Meléndez, Chiaki Kobayashi +2

We present the abundances of Li, Na, Mg, Al, Si, Ca, Sc, Ti, V, Cr, Mn, Co, Ni, Zn, Sr, Y, Zr, and Ba in a wide metallicity range ( [Fe/H] ). Using the differen…

astro-ph.SR2015★ 19 cited

The first high precision differential abundance analysis of Extremely Metal Poor stars

Henrique Reggiani, Jorge Meléndez, David Yong +2

Context: Studies of extremely metal-poor stars indicate that chemical abundance ratios [X/Fe] have an rms scatter as low as 0.05 dex (12 \%). It remains unclear whether this reflec…