activity
20112023
most citedThe Radial Velocity Experiment (RAVE): Fifth Data Release

514 citations · 4.4k across the 62 of their papers we have counts for

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Showing 2022Show all

11 papers · 1 filter

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.SR2022★ 203 cited

A Sun-like star orbiting a black hole

Kareem El-Badry, Hans-Walter Rix, Eliot Quataert +18

We report discovery of a bright, nearby () Sun-like star orbiting a dark object. We identified the system as a black hole candidate via its astrometri…

astro-ph.GA2022★ 42 cited

Chemical Cartography with LAMOST and Gaia Reveal Azimuthal and Spiral Structure in the Galactic Disk

Keith Hawkins

Chemical Cartography, or mapping, of our Galaxy has the potential to fully transform our view of its structure and formation. In this work, we use chemical cartography to explore t…

astro-ph.SR2022★ 21 cited

The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars

Z. G. Maas, K. Hawkins, N. R. Hinkel +3

Phosphorus (P) is a critical element for life on Earth yet the cosmic production sites of P are relatively uncertain. To understand how P has evolved in the solar neighborhood, we…

astro-ph.GA2022★ 28 cited

Carbon-Enhanced Metal-Poor star candidates from BP/RP Spectra in DR3

Madeline Lucey, Nariman Al Kharusi, Keith Hawkins +6

Carbon-enhanced metal-poor (CEMP) stars comprise almost a third of stars with [Fe/H] < --2, although their origins are still poorly understood. It is highly likely that one sub-cla…

astro-ph.GA2022★ 44 cited

Dynamically constraining the length of the Milky Way bar

Madeline Lucey, Sarah Pearson, Jason A. S. Hunt +5

We present a novel method for constraining the length of the Galactic bar using 6D phase space information to directly integrate orbits. We define a pseudo-length for the Galactic…

astro-ph.GA2022★ 11 cited

On the Hunt for the Origins of the Orphan--Chenab Stream: Detailed Element Abundances with APOGEE and Gaia

Keith Hawkins, Adrian M. Price-Whelan, Allyson A. Sheffield +8

Stellar streams in the Galactic halo are useful probes of the assembly of galaxies like the Milky Way. Many tidal stellar streams that have been found in recent years are accompani…

astro-ph.GA2022★ 24 cited

The relationship between age, metallicity, and abundances for disk stars in a simulated Milky Way galaxy

Andreia Carrillo, Melissa K. Ness, Keith Hawkins +4

Observations of the Milky Way's low- disk show that at fixed metallicity, [Fe/H], several element abundance, [X/Fe], correlate with age, with unique slopes and small scatters ar…

astro-ph.SR2022★ 11 cited

The Chemical Composition of Extreme-Velocity Stars

Henrique Reggiani, Alexander P. Ji, Kevin C. Schlaufman +5

Little is known about the origin of the fastest stars in the Galaxy. Our understanding of the Milky Way and surrounding dwarf galaxies chemical evolution history allows us to use t…

astro-ph.SR2022★ 38 cited

The detailed chemical abundance patterns of accreted halo stars from the optical to infrared

Andreia Carrillo, Keith Hawkins, Paula Jofré +3

Understanding the assembly of our Galaxy requires us to also characterize the systems that helped build it. In this work, we accomplish this by exploring the chemistry of accreted…

astro-ph.GA2022★ 9 cited

A GALAH View of the Chemical Homogeneity and Ages of Stellar Strings Identified in Gaia

Catherine Manea, Keith Hawkins, Zachary G. Maas

The advent of Gaia has led to the discovery of nearly 300 elongated stellar associations (called `strings') spanning hundreds of parsecs in length and mere tens of parsecs in width…