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2009MNRAS.400.1208P - Mon. Not. R. Astron. Soc., 400, 1208-1224 (2009/December-2)
Star clusters in the interacting galaxy system Arp 284.
PETERSON B.W., STRUCK C., SMITH B.J. and HANCOCK M.
Abstract (from CDS):
Clusters in the tidal tails of NGC 7714 are generally found to have ages less than 20 Myr, though observational limits make the significance of this result uncertain. Older clusters, though not numerous, have nearly the same spatial distribution within the imaged portion of NGC 7714 as young clusters. The cluster population in the bridge connecting the two galaxies appears to be older, but the data in this part of the system are too limited to draw firm conclusions. The ages of the giant Hii regions in NGC 7714 are generally older than those of their constituent clusters, possibly indicating that the young clusters we detect are surrounded by their dispersed predecessors.
Abstract Copyright: © 2009 The Authors. Journal compilation © 2009 RAS
Journal keyword(s): galaxies: individual (NGC 7714, NGC 7715) - galaxies: interactions - galaxies: star clusters
Nomenclature: Tables 2-3: [PSS2009] NNN (Nos 1-158), [PSS2009] nNN (Nos n01-n16). Tables 4-6: [SSN2005] A (Nos F-J) added. Fig. 1, Text: [PSS2009] feature N (Nos 1-6).
Status at CDS : All or part of tables of objects will not be ingested in SIMBAD.
Simbad objects: 26
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