Protostars & Planets V
Background Starlight Polarimetry (including spectropolarimetry)
Thermal Emission Polarimetry
- airborne, balloon, and satellite observations plus interferometric observations at mm, sub-mm, far-IR
- (finally!) understand how the field gets from the ISM to a protostar
Scattered-light Polarimetry
- facility instruments & adaptive optics, work at near-IR
- “circum-binary/circum-cluster” density structure