activity
20182026
most citedThe origin of the Gaia phase-plane spiral

137 citations · 514 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

Mixing stochasticity relinquishes evidence for magnetorotational hypernovae

Anmol Aggarwal, Ralph Schoenrich

A recent work claimed by fitting the observed elemental abundance pattern of a halo star with the total yields from single super-/hypernova events that only a magnetorotational hyp…

astro-ph.GA2026

An unexplored enrichment stochasticity and its implications for stellar abundance patterns

Anmol Aggarwal, Ralph Schoenrich

Extremely low metallicity stars are intensely studied as they take observations the closest to the very first generations of stars in the universe. Widely assumed to be enriched by…

astro-ph.GA2024★ 11 cited

Radial Wave in the Galactic Disk: New Clues to Discriminate Different Perturbations

Chengye Cao, Zhao-Yu Li, Ralph Schönrich +1

Decoding the key dynamical processes that shape the Galactic disk structure is crucial for reconstructing the Milky Way's evolution history. The second Gaia data release unveils a…

astro-ph.SR2020★ 28 cited

The K2 Galactic Archaeology Program Data Release 2: Asteroseismic results from campaigns 4, 6, & 7

Joel C. Zinn, Dennis Stello, Yvonne Elsworth +18

Studies of Galactic structure and evolution have benefitted enormously from Gaia kinematic information, though additional, intrinsic stellar parameters like age are required to bes…

astro-ph.GA2020★ 37 cited

Galactic Bar Resonances Inferred from Kinematically Hot Stars in Gaia EDR3

Daisuke Kawata, Junichi Baba, Jason A. S. Hunt +5

Using a numerical simulation of an isolated barred disc galaxy, we first demonstrate that the resonances of the inner bar structure induce more prominent features in the action spa…

astro-ph.GA2020★ 47 cited

Jeans modelling of the Milky Way's nuclear stellar disc

Mattia C. Sormani, John Magorrian, Francisco Nogueras-Lara +4

The nuclear stellar disc (NSD) is a flattened stellar structure that dominates the gravitational potential of the Milky Way at Galactocentric radii $30 \lesssim R \lesssim 300{\, \…

astro-ph.GA2019★ 110 cited

Resonance sweeping by a decelerating Galactic bar

Rimpei Chiba, Jennifer K. S. Friske, Ralph Schönrich

We provide the first quantitative evidence for the deceleration of the Galactic bar from local stellar kinematics in agreement with dynamical friction by a typical dark matter halo…

astro-ph.GA2019★ 26 cited

The Tilt of the Local Velocity Ellipsoid as Seen by Gaia

A. Everall, N. W. Evans, V. Belokurov +1

The Gaia Radial Velocity Spectrometer (RVS) provides a sample of 7,224,631 stars with full six-dimensional phase space information. Bayesian distances of these stars are available…

astro-ph.GA2019★ 43 cited

The chemical evolution of r-process elements from neutron star mergers: the role of a 2-phase interstellar medium

Ralph Schönrich, David H. Weinberg

Neutron star mergers (NM) are a plausible source of heavy r-process elements such as Europium, but previous chemical evolution models have either failed to reproduce the observed E…

astro-ph.GA2018★ 137 cited

The origin of the Gaia phase-plane spiral

James Binney, Ralph Schoenrich

A simple model is presented of the formation of the spiral the (z,v_z) phase plane of solar-neighbourhood stars that was recently discovered in Gaia data. The key is that the frequ…

astro-ph.GA2018★ 75 cited

Two chemically similar stellar overdensities on opposite sides of the plane of the Galaxy

Maria Bergemann, Branimir Sesar, Judith G. Cohen +9

Our Galaxy is thought to have undergone an active evolutionary history dominated by star formation, the accretion of cold gas, and, in particular, mergers up to 10 gigayear ago. Th…