Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986atsir1462....1k&link_type=abstract
Astronomicheskii Tsirkulyar NO. 1462/OCT, 1986
Astronomy and Astrophysics
Astronomy
Scientific paper
The dependence of the kinematic age of stellar groups on the value of angular velocity of the galactic spiral pattern is numerically investigated. The change of Ωp from 13 to 23 km s-1kpc-1 increases the kinematic age of stellar groups from 7×108 to 4×109years. The existence of old stellar groups (T ≡ 5×109years) in the neighbourhood of the Sun confirms values of Ωp ≡ 23 - 25 km s-1kpc-1.
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