Kinematics and chemical properties of stellar populations in the main meridional section of the Galaxy

Details Kinematics and chemical properties of stellar populations in the main meridional section of the Galaxy Kinematics and chemical properties of stellar populations in the main meridional section of the Galaxy

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mao....2e....3a&link_type=abstract

Preprint of the Main Astronomical Observatory of Academy of Sciences of Ukraine, MAO-92-2E, Kiev, p. 3-13

Astronomy and Astrophysics

Astronomy

Scientific paper

On the basis of observational data of the programme of the Galaxy main meridional section (MEGA) the stellar kinematic characteristics (rotation velocity around Galaxy Z-axis, velocity dispersions, Galaxy orbit eccentricities) with change of the z-distance and the abudance [Fe/H] and the correlation of the space density of the thin disk, thick disk, and galo stellar populations (0.98:0.02:0.003) are determined.

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