When and Why Do Star Clusters Form in the Tidal Tails of Merging Galaxies?

Details When and Why Do Star Clusters Form in the Tidal Tails of Merging Galaxies? When and Why Do Star Clusters Form in the Tidal Tails of Merging Galaxies?

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21334401c&link_type=abstract

American Astronomical Society, AAS Meeting #213, #344.01; Bulletin of the American Astronomical Society, Vol. 41, p.479

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Scientific paper

We present a survey of the tidal debris in 12 merging pairs of galaxies. Our goal was to detect super star clusters in the debris using our V and I band images from the Wide Field Planetary Camera 2 (WFPC2) on the Hubble Space Telescope. The sample of interactions includes a diverse population of tail lengths, gas mass, and both major and minor mergers and populates the entire Toomre merger sequence. We find significant populations of super star clusters in several tails, but not in the others. We discuss how star cluster formation in this environment may relate to other properties of the merger.

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