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Observational Test of an Accretion Model of Star Formation in Galactic Clusters

โœ Scribed by J. N. Pramanik; S. K. Bhattacharjee


Publisher
Springer Netherlands
Year
2006
Tongue
English
Weight
491 KB
Volume
306
Category
Article
ISSN
0004-640X

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โœ Pavel Kroupa; Monika G. Petr; Mark J. McCaughrean ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 440 KB

The frequency of low-mass pre-main sequence binary systems is significantly lower in the Trapezium Cluster than in Taurus-Auriga. We investigate if this difference can be explained through stellar encounters in dense clusters. To this effect, a range of possible models of the well observed Trapezium