activity
20182024
most citedThe Mantis Network III: Expanding the limits of chemical searches within ultra hot-Jupiters. New detections of Ca I, V I, Ti I, Cr I, Ni I, Sr II, Ba II, and Tb II in KELT-9 b

44 citations · 197 across the 10 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2024★ 5 cited

A Wide Metallicity Range for Gyr-old Stars in the Nuclear Star Cluster

Brian Thorsbro, Rebecca Forsberg, Georges Kordopatis +6

We report metallicities for three Gyr-old stars in the Milky Way nuclear star cluster (NSC) using high-resolution near-infrared spectroscopy. We derive effective temperatures…

astro-ph.GA2024

M Giants with IGRINS III. Abundance Trends for 21 Elements in the Solar Neighborhood from High-Resolution, Near-Infrared Spectra

G. Nandakumar, N. Ryde, R. Forsberg +4

In order to investigate the chemical history of the entire MilkyWay, it is imperative to also study the dust-obscured regions, where most of the mass lies. The Galactic Center is a…

astro-ph.GA2022★ 19 cited

Chemical Evolution of Ytterbium in the Galactic Disk

M. Montelius, R. Forsberg, N. Ryde +8

Measuring the abundances of neutron-capture elements in Galactic disk stars is an important part of understanding key stellar and galactic processes. In the optical wavelength regi…

astro-ph.GA2020★ 32 cited

Fluorine in the solar neighbourhood: the need for several cosmic sources

Nils Ryde, Henrik Jönsson, Gregory Mace +14

The cosmic origin of fluorine is still not well constrained. Several nucleosynthetic channels at different phases of stellar evolution have been suggested, but these must be constr…

astro-ph.GA2019★ 30 cited

Modelling the chemical evolution of Zr, La, Ce and Eu in the Galactic discs and bulge

V. Grisoni, G. Cescutti, F. Matteucci +3

We study the chemical evolution of Zr, La, Ce and Eu in the Milky Way discs and bulge by means of chemical evolution models compared with recent spectroscopic data. We consider det…

astro-ph.GA2019★ 43 cited

Abundances of disk and bulge giants from high-resolution optical spectra -- IV. Zr, La, Ce, Eu

Rebecca Forsberg, Henrik Jönsson, Nils Ryde +1

Stellar mass and metallicity are factors that affect the neutron-capture process. Due to this, the enrichment of the ISM and the abundance of neutron-capture elements vary with tim…