activity
20032026
most citedThe Radial Velocity Experiment (RAVE): first data release

939 citations · 12.8k across the 161 of their papers we have counts for

collaborators
Showing 2013Show all

7 papers · 1 filter

astro-ph.GA2013★ 213 cited

Chemodynamics of the Milky Way. I. The first year of APOGEE data

F. Anders, C. Chiappini, B. X. Santiago +38

We investigate the chemo-kinematic properties of the Milky Way disc by exploring the first year of data from the Apache Point Observatory Galactic Evolution Experiment (APOGEE), an…

astro-ph.GA2013★ 83 cited

In the thick of it: metal-poor disc stars in RAVE

G. Kordopatis, G. Gilmore, R. F. G. Wyse +17

By selecting in the RAVE-DR4 survey the stars located between 1 and 2 kpc above the Galactic plane, we question the consistency of the simplest three-component model (thin disc, th…

astro-ph.GA2013★ 93 cited

A new stellar chemo-kinematic relation reveals the merger history of the Milky Way disc

I. Minchev, C. Chiappini, M. Martig +27

The velocity dispersions of stars near the Sun are known to increase with stellar age, but age can be difficult to determine so a proxy like the abundance of alpha elements (e.g.,…

astro-ph.GA2013★ 387 cited

The RAdial Velocity Experiment (RAVE): Fourth data release

G. Kordopatis, G. Gilmore, M. Steinmetz +48

We present the stellar atmospheric parameters (effective temperature, surface gravity, overall metallicity), radial velocities, individual abundances and distances determined for 4…

astro-ph.GA2013★ 135 cited

Constraints on the Galactic Bar from the Hercules stream as traced with RAVE across the Galaxy

T. Antoja, A. Helmi, W. Dehnen +20

Non-axisymmetries in the Galactic potential (spiral arms and bar) induce kinematic groups such as the Hercules stream. Assuming that Hercules is caused by the effects of the Outer…

astro-ph.GA2013★ 75 cited

A Vertical Resonance Heating Model for X- or Peanut-Shaped Galactic Bulges

Alice C. Quillen, Ivan Minchev, Sanjib Sharma +2

We explore a second order Hamiltonian vertical resonance model for X-shaped or peanut-shaped galactic bulges. The X-shape is caused by the 2:1 vertical Lindblad resonance with the…