Wj. Maciel, SPACE DISTRIBUTION AND METALLICITIES OF GLOBULAR-CLUSTERS - THE DISTANCE TO THE GALACTIC-CENTER, Astrophysics and space science, 206(2), 1993, pp. 285-300
The system of globular clusters in the Galaxy is used in order to loca
te the position of the galactic centre and, consequently, to determine
the galacto-centric distance of the Sun, R0. The space distribution a
nd metallicities of the whole sample of known globular clusters are ta
ken into account, and the obtained results indicate that 8.6 > R0 (kpc
) > 6.4. Analysis of a selected sample of clusters further suggests th
at R0 = 7.6 +/- 0.4 kpc.