output
20032026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations

Showing 2020 · astro-ph.GAShow all

123 papers · 2 filters

astro-ph.GA2020★ 22 cited

First Co-spatial Comparison of Stellar, Neutral-, and Ionized-gas Metallicities in a metal-rich galaxy: M83

Svea Hernandez, Alessandra Aloisi, Bethan L. James +14

We carry out a comparative analysis of the metallicities from the stellar, neutral-gas, and ionized-gas components in the metal-rich spiral galaxy M83. We analyze spectroscopic obs…

astro-ph.GA2020★ 11 cited

Multiple populations in low mass globular clusters: Palomar 13

Baitian Tang, Yue Wang, Ruoyun Huang +7

Since the discovery of chemically peculiar stars in globular clusters in the last century, the study of multiple populations has become increasingly important, given that chemical…

astro-ph.GA2020★ 11 cited

A Comparison of Star-Forming Clumps and Tidal Tails in Local Mergers and High Redshift Galaxies

Debra Meloy Elmegreen, Bruce G. Elmegreen, Bradley C. Whitmore +8

The Clusters, Clumps, Dust, and Gas in Extreme Star-Forming Galaxies (CCDG) survey with the Hubble Space Telescope includes multi-wavelength imaging of 13 galaxies less than 100 Mp…

astro-ph.GA2020★ 46 cited

The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies

Myoungwon Jeon, Volker Bromm, Gurtina Besla +2

CEMP-no stars, a subset of carbon enhanced metal poor (CEMP) stars ( and ) have been discovered in ultra-faint dwarf (UFD) galaxies, with $…

astro-ph.GA2020★ 10 cited

Two Populations of Carbon-Enhanced Metal-Poor Stars in the Disk System of the Milky Way

Sarah E. Dietz, Jinmi Yoon, Timothy C. Beers +2

We present a chemo-dynamical analysis of low-resolution () spectroscopy of stars from the AAOmega Evolution of Galactic Structure (AEGIS) survey, focusing on two key p…

astro-ph.GA2020★ 14 cited

Difference in chemical composition between the bright and faint red clump stars in the Milky Way bulge

Dongwook Lim, Young-Wook Lee, Andreas Koch +7

The double red clump (RC) observed in color-magnitude diagrams of the Milky Way bulge is at the heart of the current debate on the structure and formation origin of the bulge. This…