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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 | Affiliation: | Arcetri), A.I. Sargent (Caltech), L. Olmi (LMT & FCRAO), J.S. Onello (Cortland | Abstract: | We 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 | Services: | Forum | Review | PDF | Favorites |
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