activity
20182022
most citedThe Active Chromospheres of Lithium-Rich Red Giant Stars

20 citations · 85 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202220 cited

The Active Chromospheres of Lithium-Rich Red Giant Stars

Christopher Sneden, Melike Afsar, Zeynep Bozkurt +17

We have gathered near-infrared -band high resolution spectra of nearly 300 field red giant stars with known lithium abundances in order to survey their \species{He}{i} 1083…

astro-ph.SR202010 cited

Chemical Compositions of Red Giant Stars from Habitable Zone Planet Finder Spectroscopy

Christopher Sneden, Melike Afsar, Zeynep Bozkurt +15

We have used the Habitable Zone Planet Finder (HPF) to gather high resolution, high signal-to-noise near-infrared spectra of 13 field red horizontal-branch (RHB) stars, one open-cl…

astro-ph.SR201919 cited

Chemical Abundances Of Open Clusters From High-Resolution Infrared Spectra. II. NGC 752

G. Böcek Topcu, M. Afsar, C. Sneden +9

We present a detailed near-infrared chemical abundance analysis of 10 red giant members of the Galactic open cluster NGC 752. High-resolution (R45000) near-infrared spectra…

astro-ph.SR201918 cited

The chemical compositions and evolutionary status of red giants in the open cluster NGC 6940

G. Böcek Topcu, M. Afşar, C. Sneden

We present the high resolution (R 60000), high signal-to-noise (S/N 120) spectroscopic analysis of 12 red giant members of the Galactic open cluster NGC 6940. We…

astro-ph.SR201918 cited

Chemical Abundances Of Open Clusters From High-Resolution Infrared Spectra. I. NGC 6940

G. Böcek Topcu, M. Afsar, C. Sneden +8

We present near-infrared spectroscopic analysis of 12 red giant members of the Galactic open cluster NGC 6940. High-resolution (R45000) and high signal-to-noise ratio (S/N…

astro-ph.SR2018

Chemical Compositions of Evolved Stars From Near-Infrared IGRINS High-Resolution Spectra. I. Abundances in Three Red Horizontal Branch Stars

Melike Afşar, Christopher Sneden, Michael P. Wood +6

We have derived elemental abundances of three field red horizontal branch stars using high-resolution (R 45,000), high signal-to-noise ratio (S/N 200) and