activity
20202026
most citedEvidence from APOGEE for the presence of a major building block of the halo buried in the inner Galaxy

224 citations · 1.2k across the 65 of their papers we have counts for

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Showing 2024Show all

17 papers · 1 filter

astro-ph.GA2024★ 3 cited

A slow spin to win -- the gradual evolution of the proto-Galaxy to the old disc

Akshara Viswanathan, Danny Horta, Adrian M. Price-Whelan +1

Observational studies are identifying stars thought to be remnants from the earliest stages of the hierarchical mass assembly of the Milky Way, referred to as the proto-Galaxy. We…

astro-ph.SR2024

Evidence of Truly Young high- Dwarf Stars

Yuxi Lu, Isabel L. Colman, Maryum Sayeed +14

The existence of high- stars with inferred ages < 6 Gyr has been confirmed recently with large spectroscopic and photometric surveys. However, stellar mergers or binary interact…

astro-ph.GA2024★ 1 cited

Modelling the density and mass of the Milky Way's proto-galaxy components with -

Danny Horta, Ricardo P. Schiavon

Unravelling galaxy formation theory requires understanding galaxies both at high and low redshifts. A possible way to connect both realms is by studying the oldest stars in the Mil…

astro-ph.GA2024

Cosmological predictions for minor axis stellar density profiles in the inner regions of Milky Way-mass galaxies

Madeline Lucey, Robyn Sanderson, Danny Horta +5

CDM cosmology predicts the hierarchical formation of galaxies which build up mass by merger events and accreting smaller systems. The stellar halo of the Milky Way has proven to…

astro-ph.GA2024

2-process Model and Residual Abundance Analysis of the Milky Way Massive Satellites

Sten Hasselquist, Christian R. Hayes, Emily J. Griffith +4

The ``2-process Model'' is a promising technique for interpreting stellar chemical abundance data from large-scale surveys (e.g., SDSS-IV/V, GALAH), enabling more quantitative empi…

astro-ph.GA2024★ 6 cited

Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?

Dylan Folsom, Mariangela Lisanti, Lina Necib +3

Observations of the Milky Way's stellar halo find that it is predominantly comprised of a radially biased population of stars, dubbed the Gaia Sausage--Enceladus, or GSE. These sta…

astro-ph.GA2024★ 1 cited

The Extremely Metal Rich Knot of Stars at the Heart of the Galaxy

Hans-Walter Rix, Vedant Chandra, Gail Zasowski +15

We show with Gaia XP spectroscopy that extremely metal-rich stars in the Milky Way (EMR; ) - but only those - are largely confined to a tight "knot" at the center…

astro-ph.GA2024★ 5 cited

The imprint of dark matter on the Galactic acceleration field

Arpit Arora, Robyn E. Sanderson, Sukanya Chakrabarti +6

Measurements of the accelerations of stars enabled by time-series extreme-precision spectroscopic observations, from pulsar timing, and from eclipsing binary stars in the Solar Nei…

astro-ph.GA2024★ 1 cited

[X/Fe] Marks the Spot: Mapping Chemical Azimuthal Variations in the Galactic Disk with APOGEE

Zoe Hackshaw, Keith Hawkins, Carrie Filion +4

Chemical cartography of the Galactic disk provides insights to its structure and assembly history over cosmic time. In this work, we use chemical cartography to explore chemical gr…

astro-ph.GA2024

On the mass assembly history of the Milky Way: clues from its stellar halo

Danny Horta, Ricardo P. Schiavon

Stellar halos of galaxies retain crucial clues to their mass assembly history. It is in these galactic components that the remains of cannibalised galactic building blocks are depo…

astro-ph.GA2024★ 1 cited

Stellar Mergers or Truly Young? Intermediate-Age Stars on Highly-Radial Orbits in the Milky Way's Stellar Halo

Danny Horta, Yuxi, Lu +3

Reconstructing the mass assembly history of the Milky Way relies on obtaining detailed measurements of the properties of many stars in the Galaxy, especially in the stellar halo. O…

astro-ph.GA2024★ 7 cited

Measuring Dwarf Galaxy Intrinsic Abundance Scatter with Mid-resolution Spectroscopic Surveys: Calibrating APOGEE Abundance Errors

Jennifer Mead, Melissa Ness, Eric Andersson +2

The first generations of stars left their chemical fingerprints on metal-poor stars in the Milky Way and its surrounding dwarf galaxies. While instantaneous and homogeneous enrichm…

astro-ph.GA2024★ 1 cited

Disentangling the Galaxy's Gordian knot: evidence from for a knotted and slower bar in the Milky Way

Danny Horta, Michael S. Petersen, Jorge Peñarrubia

The inner kiloparsec (kpc) region of the Milky Way is complex. Unravelling the evolution of the Galaxy requires precise understanding of the formation of this region. We re…

astro-ph.GA2024

A perspective on the Milky Way Bulge-Bar as seen from the neutron-capture elements Cerium and Neodymium with APOGEE

J. V. Sales-Silva, K. Cunha, V. V. Smith +28

This study probes the chemical abundances of the neutron-capture elements cerium and neodymium in the inner Milky Way from an analysis of a sample of 2000 stars in the Galact…

astro-ph.GA2024★ 16 cited

Radial phase spirals in the Solar neighbourhood

Jason A. S. Hunt, Adrian M. Price-Whelan, Kathryn V. Johnston +4

The second data release of ESA's mission revealed numerous signatures of disequilibrium in the Milky Way's disc. These signatures are seen in the planar kinematics of stars,…

astro-ph.GA2024★ 1 cited

Data-driven Dynamics with Orbital Torus Imaging: A Flexible Model of the Vertical Phase Space of the Galaxy

Adrian M. Price-Whelan, Jason A. S. Hunt, Danny Horta +4

The vertical kinematics of stars near the Sun can be used to measure the total mass distribution near the Galactic disk and to study out-of-equilibrium dynamics. With contemporary…

astro-ph.SR2024

Spectacular nucleosynthesis from early massive stars

Alexander P. Ji, Sanjana Curtis, Nicholas Storm +39

Stars formed with initial mass over 50 Msun are very rare today, but they are thought to be more common in the early universe. The fates of those early, metal-poor, massive stars a…