most citedHigh-Resolution Infrared Spectroscopy of the Dust-Obscured Metal-Poor Open Cluster Trumpler 5

3 citations · 6 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA2025

Rubidium Abundances in Cool Giants from High-Resolution H-band Spectra: A New Diagnostic for Galactic Chemical Evolution

Nils Ryde, Jess Kocher, Govind Nandakumar +6

The Galactic Center and inner disk of the Milky Way contain complex stellar populations obscured by heavy dust extinction. To study their chemical composition, high-resolution near…

astro-ph.GA2025

The First Chemical Census the Milky Way's Nuclear Star Cluster

Govind Nandakumar, Nils Ryde, Mathias Schultheis +4

An important step in understanding the formation and evolution of the Nuclear Star Cluster (NSC) is to investigate its chemistry and chemical evolution. Additionally, exploring the…

astro-ph.GA2024

Chemical Abundances in the Nuclear Star Cluster of the Milky Way: alpha-Element Trends and Their Similarities with the Inner Bulge

N. Ryde, G. Nandakumar, M. Schultheis +15

A chemical characterization of the Galactic Center is essential for understanding its formation and structural evolution. Trends of alpha-elements, such as Mg, Si, and Ca, serve as…

astro-ph.GA20243 cited

M giants with IGRINS IV. Identification and characterization of a near-IR line of the s-element Barium

G. Nandakumar, N. Ryde, H. Hartman +1

Neutron-capture elements represent an important nucleosynthetic channel in the study of the Galactic Chemical Evolution of stellar populations. For stellar populations behind signi…

astro-ph.GA2024

Composition of Giants 1 North of the Galactic Center: Detailed Abundance Trends for 21 Elements Observed with IGRINS

Govind Nandakumar, Nils Ryde, Gregory Mace +10

We report the first high resolution, detailed abundances of 21 elements for giants in the Galactic bulge/bar within of the Galactic plane, where high extinction has rende…

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…