Kinematics of the Milky Way from the Gaia EDR3 red giants and sub-giants
PN Fedorov, VS Akhmetov, AB Velichko… - arXiv preprint arXiv …, 2021
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 …
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 …
| • | Перше бібліографічне посиланняKinematics of main-sequence … |

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