Abstract
We have analyzed HST/WFPC2 images of NGC 3597 and find ≃700 compact objects surrounding the galaxy with an average (B-R)o ≃ 0.6. We propose that the majority of these objects are young globular clusters. They have a spread in colors that is consistent with that expected for a population of young clusters with a common age and spread induced by photometric errors and reddening within NGC 3597. If these objects were similar to the Galactic globular cluster system seen at a younger age, we would predict a turnover in the luminosity function at B ≃ 23. However, we find that the luminosity function for the clusters is increasing to the limits of our photometry (B ≃ 27).
Original language | English |
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Pages (from-to) | 1700-1707 |
Number of pages | 8 |
Journal | Astronomical Journal |
Volume | 117 |
Issue number | 4 |
DOIs | |
Publication status | Published - Apr 1999 |