The Existence of the Third Integral for a Family of High-Velocity Stars

Details The Existence of the Third Integral for a Family of High-Velocity Stars The Existence of the Third Integral for a Family of High-Velocity Stars

Apr 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...7..139i&link_type=abstract

Astrophysics and Space Science, Volume 7, Issue 1, pp.139-150

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A family of high-velocity stars (Energy-19000
km2/sec2, angular momentum 1150 kpc km/sec) were
computed using Innanen's (1966) mass model of the Galaxy. The stars were
set initially on the curve of zero velocity. The inclination diagram
indicates a quasi-isolating third integral.

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