STAR CLUSTERS IN THE NEARBY LATE-TYPE GALAXY NGC 1311
Journal Article
·
· Astronomical Journal (New York, N.Y. Online)
- Department of Physics and Astronomy, Minnesota State University, Mankato, MN 56001 (United States)
- Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH (United Kingdom)
- Sterrenkundig Instituut, Universiteit Utrecht, NL-3508 TA Utrecht (Netherlands)
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287 (United States)
Ultraviolet, optical and near-infrared images of the nearby (D {approx} 5.5 Mpc) SBm galaxy NGC 1311, obtained with the Hubble Space Telescope, reveal a small population of 13 candidate star clusters. We identify candidate star clusters based on a combination of their luminosity, extent, and spectral energy distribution. The masses of the cluster candidates range from {approx}10{sup 3} M{sub sun} up to {approx}10{sup 5} M{sub sun}, and show a strong positive trend of larger mass with increasing with cluster age. Such a trend follows from the fading and dissolution of old, low-mass clusters, and the lack of any young super-star clusters of the sort often formed in strong starbursts. The cluster age distribution is consistent with a bursting mode of cluster formation, with active episodes of age {approx}10 Myr, {approx}100 Myr, and {approx}>Gyr. The ranges of age and mass we probe are consistent with those of the star clusters found in quiescent Local Group dwarf galaxies.
- OSTI ID:
- 21583029
- Journal Information:
- Astronomical Journal (New York, N.Y. Online), Journal Name: Astronomical Journal (New York, N.Y. Online) Journal Issue: 1 Vol. 135; ISSN 1538-3881
- Country of Publication:
- United States
- Language:
- English
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