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20182020
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astro-ph.GA2019

Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18

F. Anders, A. Khalatyan, C. Chiappini +19

Combining the precise parallaxes and optical photometry delivered by Gaia's second data release (Gaia DR2) with the photometric catalogues of PanSTARRS-1, 2MASS, and AllWISE, we de…

astro-ph.GA2019

Kinematics with Gaia DR2: The Force of a Dwarf

I. Carrillo, I. Minchev, M. Steinmetz +10

We use Gaia DR2 astrometric and line-of-sight velocity information combined with two sets of distances obtained with a Bayesian inference method to study the 3D velocity distributi…

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

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

Correlations between age, kinematics, and chemistry as seen by the RAVE survey

Jennifer Wojno, Georges Kordopatis, Matthias Steinmetz +20

We explore the connections between stellar age, chemistry, and kinematics across a Galactocentric distance of , using a sample of inte…

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…