Intergalactic Globular Clusters and the Faint End of the Galaxy Number Counts in A1656 (Coma)
The existence of an intergalactic globular cluster population in the Coma cluster of galaxies has been tested using surface brightness fluctuations. The main result is that the intergalactic globular cluster surface density (NIGC) does not correlate with the distance to the center of Coma and hence with the environment. Furthermore, comparing these
Marín-Franch, A. et al.
Fecha de publicación:
3
2003