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STAR CLUSTERS IN THE NEARBY LATE-TYPE GALAXY NGC 1311

Journal Article · · Astronomical Journal (New York, N.Y. Online)
 [1];  [2];  [3]; ;  [4]
  1. Department of Physics and Astronomy, Minnesota State University, Mankato, MN 56001 (United States)
  2. Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH (United Kingdom)
  3. Sterrenkundig Instituut, Universiteit Utrecht, NL-3508 TA Utrecht (Netherlands)
  4. 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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