activity
20172021
most citedThe age-metallicity structure of the Milky Way disk

191 citations · 554 across the 6 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.GA2019110 cited

Weighing the stellar constituents of the Galactic halo with APOGEE red giant stars

J. Ted Mackereth, Jo Bovy

The stellar mass in the halo of the Milky Way is notoriously difficult to determine, owing to the paucity of its stars in the solar neighbourhood. With tentative evidence from $\it…

astro-ph.GA2019

Searching for Solar Siblings in APOGEE and DR2 with N-body Simulations

Jeremy J. Webb, Natalie Price-Jones, Jo Bovy +4

We make use of APOGEE and data to identify stars that are consistent with being born in the same association or star cluster as the Sun. We limit our analysis to stars that…

astro-ph.GA2019

Life in the fast lane: a direct view of the dynamics, formation, and evolution of the Milky Way's bar

Jo Bovy, Henry W. Leung, Jason A. S. Hunt +3

Studies of the ages, abundances, and motions of individual stars in the Milky Way provide one of the best ways to study the evolution of disk galaxies over cosmic time. The formati…

astro-ph.GA2019

He abundances in disc galaxies -- I. Predictions from cosmological chemodynamical simulations

Fiorenzo Vincenzo, Andrea Miglio, Chiaki Kobayashi +2

We investigate how the stellar and gas-phase He abundances evolve as functions of time within simulated star-forming disc galaxies with different star formation histories. We make…

astro-ph.GA2019

Signatures of resonance and phase mixing in the Galactic disc

Jason A. S. Hunt, Mathew W. Bub, Jo Bovy +3

Gaia DR2 has provided an unprecedented wealth of information about the kinematics of stars in the Solar neighbourhood, and has highlighted the degree of features in the Galactic di…

astro-ph.GA2019

A galaxy's accretion history unveiled from its integrated spectrum

Alina Boecker, Ryan Leaman, Glenn van de Ven +3

We present a new method of quantifying a galaxy's accretion history from its integrated spectrum alone. Using full spectral fitting and calibrated regularization techniques we show…