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Polarimetry

Description:
My collaborators and I have shown that, contrary to previously prevailing ideas,
polarimetry of background starlight cannot reliably reveal the magnetic field structure
in dense interstellar clouds, because polarization efficiency is apparently low there.
Much of our work in this area revolves around quantifying what exactly *is* measurable
with background starlight polarimetry, and what other techniques for mapping field
structure can/will work better.

"Theory" - Background Starlight - Thermal Emission

"Theory"

Collaborators: Publications:

Theory
Background Starlight
Collaborators: Publications: Web Sites:
Background StarlightBackground Starlight
Thermal Emission
Collaborators: Publications: Web Sites:
M4

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Last modified on Monday, 22-Jan-2007 12:10:30 EST