Radial motion in the galactic system of globular clusters

Details Radial motion in the galactic system of globular clusters Radial motion in the galactic system of globular clusters

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979mnras.187..863c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 187, June 1979, p. 863-870.

Astronomy and Astrophysics

Astronomy

17

Astronomical Models, Galactic Nuclei, Globular Clusters, Radial Velocity, Stellar Motions, Astrometry, Astronomical Photometry, Cepheid Variables, Steady State, Velocity Distribution

Scientific paper

It is shown that the radial velocities of globular clusters close to the Galactic Center direction are not consistent with a simple steady-state model of the galactic halo. The result is unlikely to be altered significantly by subsequent improvements in distances, radial velocities, or galactic models. The noncircular motion in this line of sight corresponds to an average of about +60 km/s.

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