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19 April 2024
 
  » arxiv » astro-ph/0005522

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Star formation in clusters: early sub-clustering in the Serpens core
L. Testi ; A.I. Sargent ; L. Olmi ; J.S. Onello ;
Date 25 May 2000
Subject astro-ph
AffiliationArcetri), A.I. Sargent (Caltech), L. Olmi (LMT & FCRAO), J.S. Onello (Cortland
AbstractWe present high resolution interferometric and single dish observations of molecular gas in the Serpens cluster-forming core. Star formation does not appear to be homogeneous throughout the core, but is localised in spatially- and kinematically-separated sub-clusters. The stellar (or proto-stellar) density in each of the sub-clusters is much higher than the mean for the entire Serpens cluster. This is the first observational evidence for the hierarchical fragmentation of proto-cluster cores suggested by cluster formation models.
Source arXiv, astro-ph/0005522
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