Kinematics of the Milky Way from the Gaia EDR3 red giants and sub-giants

Abstract

We present the results of the kinematic investigations carried out with the use of spatial velocities of red giants and sub-giants containing in the $Gaia$~EDR3 catalogue. The twelve kinematic parameters of the Ogorodnikov--Milne model have been derived for stellar systems with radii 0.5 and 1.0 kpc, located along the direction the Galactic center -- the Sun -- the Galactic anticenter within the range of Galactocentric distances $R$ 0--8--16~kpc. By combining some of the local parameters the information related to the Galaxy as a whole has been received in the distance range 4--12~kpc, in particular the Galactic rotational curve, its slope, velocity gradients. We show that when using this approach, there is an alternative possibility to infer the behaviour of the Galactic rotational curve and its slope without using the Galactocentric distance $R_{\odot }$. The kinematic parameters derived within the Solar vicinity of 1~kpc radius are in good agreement with those given in literature.

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• Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
• Estimating distances from parallaxes. V: Geometric and photogeometric distances to 1.47 billion stars in Gaia Early Data Release 3
• Gaia Data Release 3 Properties and validation of the radial velocities
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Cited by in corpus (5)

• A new kinematic model of the Galaxy: analysis of the stellar velocity field from Gaia Data Release 3
• Gaussian Process Model for the Local Stellar Velocity Field from Gaia Data Release 2
• Mapping the kinematic parameters of the Galaxy from the Gaia EDR3 red giants and sub-giants
• The vertex coordinates of the Galaxy's stellar systems according to the Gaia DR3 catalogue
• Spatial orientation and shape of the velocity ellipsoids of the Gaia DR3 giants and subgiants in the Galactic plane