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Monday 17 September at 2pm

Sebastian Wolf - Thuringer Landessternwarte Tautenburg

"Alignment of Disks of TTauri Binary Stars"

ABSTRACT: "I will present the results of a study performed with the goal to investigate whether low-mass pre-main sequence binary stars are formed by multiple fragmentation or via stellar capture. If binaries form preferentially by fragmentation, their disks are expected to be co-planar. On the other hand, the capture scenario will lead to a random distribution of disk orientations. For this reason, near-infrared polarization measurements of 49 young close binary stars in the K band with SOFI at the NTT have been performed. The near-infrared excess radiation of the targets mostly point to the presence of disks. For a major fraction of the sample, evidence for disks is also obvious from other features (outflows, jets, Herbig-Haro objects). The disk orientation was derived from the orientation of the polarization vector of both components of each binary. This statistical study allows to test which hypothesis (co-planarity, random orientation) is consistent with the observed distribution of polarimetric position angles. Evidence was found that the disks are preferentially aligned."
 

Contact: Chris Davis. Updated: Tue Sep 28 12:20:53 HST 2004

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