C32, A Young Star Cluster in IC 1613
arXiv:astro-ph/0002439 · doi:10.1086/316571
Abstract
The Local Group irregular galaxy IC 1613 has remained an enigma for many years because of its apparent lack of star clusters. We report the successful search for clusters among several of the candidate objects identified many years ago on photographic plates. We have used a single HST WFPC2 pointing and a series of images obtained with the WIYN telescope under exceptional seeing conditions, examining a total of 23 of the previously published candidates. All but six of these objects were found to be either asterisms or background galaxies. Five of the six remaining candidates possibly are small, sparse clusters and the sixth, C32, is an obvious cluster. It is a compact, young object, with an age of less than 10 million years and a total absolute magnitude of M_V = -5.78+/-0.16 within a radius of 13 pc.
5 pages, 5 figures, to be published in the May 2000 issue of the PASP
References in corpus (1)
Cited by in corpus (9)
- The Luminosity Function of Star Clusters in Spiral Galaxies
- Deep Hubble Space Telescope Imaging of IC 1613 II. The Star Formation History
- Super-star clusters versus OB associations
- Young massive star clusters in M51
- Clearing the hurdle: The mass of globular cluster systems as a function of host galaxy mass
- A Spitzer IRAC Census of the Asymptotic Giant Branch Populations in Local Group Dwarfs. II. IC 1613
- Rubin Observatory LSST Stars Milky Way and Local Volume Star Clusters Roadmap
- The X-ray-Resolved Supernova Remnant S8 in the Dwarf Irregular Galaxy IC 1613
- Detection of X-ray elongated emission from a ultraluminous X-ray source in the interacting pair of galaxies NGC 5953/5954