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Special Colloquium - "Magnetic Fields in PDRs - Zeeman Effect Measurements and Their Implications"

Speaker Tom Troland, University of Kentucky
Date: 5/23/2017
Time: 3:45 p.m.
Location:

Astronomy 134

Sponsor:

Prof. Richard Crutcher

Event Type: Seminar/Symposium
 

Aperture synthesis observations of the 21cm HI Zeeman effect offer an unusual opportunity to measure magnetic field strengths in PDRs.  If a PDR lies in front of an H+ region, strong radio free-free emission can create deep HI absorption lines that are very sensitive to the Zeeman effect.   Zeeman observations have been performed toward a number of galactic H+ regions.  PDR field strengths are often quite high (up to a milligauss).  Published Cloudy PDR models of M17 describe an equilibrium between magnetic pressure and the momentum of absorbed stellar uv radiation.   This model can be applied to all H+ regions for which Zeeman measurements exist.  The model suggests that magnetic fields play a crucial role in determining PDR physical properties such as depth and density.

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