activity
20062025
most citedA Young Stellar Cluster Surrounding the Peculiar Eruptive Variable V838 Monocerotis

49 citations · 395 across the 21 of their papers we have counts for

collaborators

19 papers

astro-ph.SR2025

High Lithium Abundance Connection with the Chromospheric Helium in Red Giants: Spectroscopic and Asteroseismic analyses

Anohita Mallick, Christopher Sneden, Bacham E. Reddy +1

We present a study of correlations between high Li abundances and strong chromospheric He I 10830 Å absorption line strengths in Kepler field giant stars. Our sample includes 84 gi…

astro-ph.SR2023★ 11 cited

M67 Blue Stragglers with High-resolution Infrared Spectroscopy

K. E. Brady, C. Sneden, C. A. Pilachowski +5

We report on the first detailed infrared chemical analysis of five binary members (S277, S997, S975, S1031, and S1195) in the open cluster M67 (NGC 2682). These stars are located o…

astro-ph.SR2023★ 6 cited

Chemical Compositions of Red Giant Stars in the Old Open Cluster NGC 7789

Neel Nagarajan, Christopher Sneden, Melike Afsar +1

We have gathered optical-region spectra, derived model atmosphere parameters, and computed elemental abundances for 15 red giant stars in the open cluster NGC 7789. We focus on the…

astro-ph.SR2023★ 12 cited

Effective Temperature Estimations from Line Depth Ratios in the \H\ and \K-band Spectra of IGRINS

Melike Afşar, Zeynep Bozkurt, Gamze Böcek Topcu +5

Determining accurate effective temperatures of stars buried in the dust-obscured Galactic regions is extremely difficult from photometry. Fortunately, high-resolution infrared spec…

astro-ph.SR2022★ 20 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.GA2022★ 6 cited

Mapping the aliphatic hydrocarbon content of interstellar dust in the Galactic plane

B. Günay, M. G. Burton, M. Afşar +1

We implement a new observational method for mapping the aliphatic hydrocarbon content in the solid phase in our Galaxy, based on spectrophotometric imaging of the 3.4 m absorpti…