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Astronomy Colloquium (2019 Spring Semester)

* Date
May 16
* Speaker
Dr. Pei-Ying Hsieh (ASIAA)
* Title
The Role of the Magnetic Field in the Circumnuclear Disk of the Galactic Center – Implications From 850 micron Polarization Data
* Abstract
 

 

Utilizing James Clark Maxwell Telescope (JCMT) 850 micron SCUPOL dust polarization data, we investigate the configuration of the magnetic (B-) field in the circumnuclear disk (CND) of the Galactic Center (GC). Overall on a large scale, the B-field shows a clear predominantly toroidal morphology. Compared to earlier 100 micron and 350 micron observations, the SCUPOL data show a largely improved polarization coverage at a higher resolution. In general, the observed
B-field morphology is well described by a self-similar axisymmetric disk model where the radial infall velocity is one quarter of the rotational velocity. A detailed comparison with higher-resolution interferometric maps from the Submillimeter Array (SMA) further reveals that the B-field aligns with the neutral gas streamers where they are connecting to the CND. Moreover, the innermost observed B-field structure also appears to trace and align with the ionized mini-spirals located inside the CND. This suggests that there might be one underlying B-field structure that is connecting the CND with its streamers and the inner mini-spirals. An estimate of beta plasma parameter ~1 – based on the global B-field morphology that constrains the azimuthal-to-vertical field strength ratio to be around 40 combined with a measurement of the azimuthal velocity — indicates that the B-field appears dynamically significant towards the CND and also onwards to the inner mini-spirals.
 
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