Proceedings of the
Workshop
"
The Magellanic Clouds and Other Dwarf Galaxies"
of the
Bonn/Bochum-Graduiertenkolleg
The Formation and Evolution of Rich Star Clusters in the LMC:
NGC 1818
Rebecca A. W. Elson, Gerard Gilmore, Sverre Aarseth, Melvyn Davies,
Steinn Sigurdsson, Basilio Santiago, and Jarrod Hurley
Fig. 1.
Colour-magnitude diagram for objects detected in the PC image
(the central ∼ 2 rc) of NGC 1818.
A binary sequence is clearly visible.
At V555 < ∼ 17.5 the stars are saturated.
The dashed lines indicate the magnitude limits of our sample
Links (back/forward) to:
| First version: | 19th | February, | 1998
|
| Last update: | 29th | September, | 1998
|
Jochen M. Braun &
Tom Richtler
(E-Mail: jbraun|richtler@astro.uni-bonn.de)