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19992023
most citedThe Galactic Thick Disk Stellar Abundances

422 citations · 4.4k across the 64 of their papers we have counts for

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14 papers · 1 filter

astro-ph.SR2023

Metallicities of Classical Cepheids in the Inner Galactic Disk

N. Matsunaga, D. Taniguchi, S. S. Elgueta +14

Metallicity gradients refer to the sloped radial profile of metallicities of gas and stars and are commonly seen in disk galaxies. A well-defined metallicity gradient of the Galact…

astro-ph.SR2020★ 18 cited

A "blue ring nebula" surrounding a thousands of years old stellar merger

Keri Hoadley, Christopher Martin, Brian D. Metzger +7

Stellar mergers are a brief-lived but common phase in the evolution of binary star systems. Among the many astrophysical implications of these events include the creation of atypic…

astro-ph.SR2020★ 17 cited

A high-precision abundance analysis of the nuclear benchmark star HD 20

Michael Hanke, Camilla Juul Hansen, Hans-Günter Ludwig +4

We present our chemical abundance investigation of the metal-poor ([Fe/H]=-1.60 dex), r-process-enriched ([Eu/Fe]=0.73 dex) halo star HD 20 using novel and archival high-resolution…

astro-ph.SR2020★ 34 cited

The Cluster Ages Experiment (CASE). VIII. Age and Distance of the Globular Cluster 47 Tuc from the Analysis of Two Detached Eclipsing Binaries

I. B. Thompson, A. Udalski, A. Dotter +20

We use photometric and spectroscopic observations of the eclipsing binary E32 in the globular cluster 47 Tuc to derive the masses, radii, and luminosities of the component stars. T…

astro-ph.SR2019★ 32 cited

A Reanalysis of the Fundamental Parameters and Age of TRAPPIST-1

Eileen C. Gonzales, Jacqueline K. Faherty, Jonathan Gagné +3

We present the distance-calibrated spectral energy distribution (SED) of TRAPPIST-1 using a new medium resolution (R~6000) near-infrared FIRE spectrum and its Gaia parallax. We rep…

astro-ph.SR2019★ 69 cited

Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies

Evan N. Kirby, Justin L. Xie, Rachel Guo +6

There is no consensus on the progenitors of Type Ia supernovae (SNe Ia) despite their importance for cosmology and chemical evolution. We address this question by using our previou…