We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (RAVE) and Geneva-Copenhagen Survey (GCS) stellar surveys. We do this by fitting a kinematic model to the data and taking the selection function of the data into account. For stars in the GCS we use all phase-space coordinates, but for RAVE stars we use only (l, b, v los). Using the Markov Chain Monte Carlo technique, we investigate the full posterior distributions of the parameters given the data. We investigate the age-velocity dispersion relation for the three kinematic components (σ R , σphi, σ z ), the radial dependence of the velocity dispersions, the solar peculiar motion (U ⊙, V ⊙, W ⊙), the circular speed Θ0 at the Sun, and the fall o...
We analyze the distribution of G and K type stars towards the Galactic poles using RAVE and ELODIE r...
We analyse the kinematics of ˜400 000 stars that lie within ˜2 kpc of the Sun and have spectra measu...
International audienceAims. We attempt to constrain the kinematics of the thin and thick disks using...
We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (...
We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (...
We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (...
© 2014. The American Astronomical Society. All rights reserved.. We investigate the kinematic parame...
We analyse the kinematics of ~400000 RAVE stars. We split the sample into hot and cold dwarfs, red-c...
We analyze the distribution of G and K type stars towards the Galactic poles using RAVE and ELODIE r...
Aims. We study the Milky Way (MW) thin disk with the RAdial Velocity Experiment (RAVE) survey. We co...
We study the kinematics of the Galactic thin and thick disk populations us-ing stars from the RAVE s...
We analyse the kinematics of ~400 000 stars that lie within ̃2 kpc of the Sun and have spectra measu...
Context. Radial velocity surveys such as the RAdial Velocity Experiment (RAVE) provide us with measu...
We analyse the kinematics of ∼400 000 stars that lie within ∼2 kpc of the Sun and have spectra measu...
Aims. We attempt to constrain the kinematics of the thin and thick disks using the Besançon populati...
We analyze the distribution of G and K type stars towards the Galactic poles using RAVE and ELODIE r...
We analyse the kinematics of ˜400 000 stars that lie within ˜2 kpc of the Sun and have spectra measu...
International audienceAims. We attempt to constrain the kinematics of the thin and thick disks using...
We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (...
We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (...
We investigate the kinematic parameters of the Milky Way disk using the Radial Velocity Experiment (...
© 2014. The American Astronomical Society. All rights reserved.. We investigate the kinematic parame...
We analyse the kinematics of ~400000 RAVE stars. We split the sample into hot and cold dwarfs, red-c...
We analyze the distribution of G and K type stars towards the Galactic poles using RAVE and ELODIE r...
Aims. We study the Milky Way (MW) thin disk with the RAdial Velocity Experiment (RAVE) survey. We co...
We study the kinematics of the Galactic thin and thick disk populations us-ing stars from the RAVE s...
We analyse the kinematics of ~400 000 stars that lie within ̃2 kpc of the Sun and have spectra measu...
Context. Radial velocity surveys such as the RAdial Velocity Experiment (RAVE) provide us with measu...
We analyse the kinematics of ∼400 000 stars that lie within ∼2 kpc of the Sun and have spectra measu...
Aims. We attempt to constrain the kinematics of the thin and thick disks using the Besançon populati...
We analyze the distribution of G and K type stars towards the Galactic poles using RAVE and ELODIE r...
We analyse the kinematics of ˜400 000 stars that lie within ˜2 kpc of the Sun and have spectra measu...
International audienceAims. We attempt to constrain the kinematics of the thin and thick disks using...