activity
20132022
most citedPainting a portrait of the Galactic disc with its stellar clusters

554 citations · 2.2k across the 19 of their papers we have counts for

collaborators
Showing 2018Show all

6 papers · 1 filter

astro-ph.GA2018

The escape speed curve of the Galaxy obtained from Gaia DR2 implies a heavy Milky Way

Giacomo Monari, Benoit Famaey, Ismael Carrillo +6

We measure the escape speed curve of the Milky Way based on the analysis of the velocity distribution of counter-rotating halo stars from the Gaia DR2. The distances we…

astro-ph.GA2018

The metal-rich halo component extended in z: a characterization with Gaia DR2 and APOGEE

Emma Fernández-Alvar, J. G. Fernández-Trincado, Edmundo Moreno +12

We report an analysis of the metal-rich tail ([Fe/H] ) of halo stars located at distances from the Galactic plane up to kpc, observed by the Apache Point…

astro-ph.GA2018

Spiral arm crossings inferred from ridges in Gaia stellar velocity distributions

Alice C. Quillen, Ismael Carrillo, Friedrich Anders +7

The solar neighborhood contains disc stars that have recently crossed spiral arms in the Galaxy. We propose that boundaries in local velocity distributions separate stars that have…

astro-ph.GA2018

Estimating stellar birth radii and the time evolution of the Milky Way's ISM metallicity gradient

I. Minchev, F. Anders, A. Recio-Blanco +14

We present a semi-empirical, largely model-independent approach for estimating Galactic birth radii, r_birth, for Milky Way disk stars. The technique relies on the justifiable assu…

astro-ph.SR2018

Chemo-kinematics of the Milky Way from the SDSS-III MARVELS Survey

Nolan Grieves, Jian Ge, Neil Thomas +20

Combining stellar atmospheric parameters, such as effective temperature, surface gravity, and metallicity, with barycentric radial velocity data provides insight into the chemo-dyn…

astro-ph.GA2018

Dissecting stellar chemical abundance space with t-SNE

Friedrich Anders, Cristina Chiappini, Basílio X. Santiago +4

In the era of industrial Galactic astronomy and multi-object spectroscopic stellar surveys, the sample sizes and the number of available stellar chemical abundances have reached di…