A New Mechanism for Polarizing Light from Obscured Stars
arXiv:0708.0599 · doi:10.1086/522425
Abstract
Recent spectropolarimetric observations of Herbig AeBe stellar systems show linear polarization variability with wavelength and epoch near their obscured H-alpha emission. Surprisingly, this polarization is not coincident with the H-alpha emission peak but is variable near the absorptive part of the line profile. With a new and novel model we show here that this is evidence of optical pumping - anisotropy of the incident radiation that leads to a linear polarization-dependent optical depth within the intervening hydrogen wind or disk cloud. This effect can yield a larger polarization signal than scattering polarization in these systems.
Submitted to ApJ Letters
References in corpus (3)
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- Spectropolarimetric observations of Herbig Ae/Be Stars I: HiVIS spectropolarimetric calibration and reduction techniques
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- Linear spectropolarimetry across the optical spectrum of Herbig Ae/Be stars
- Linear line spectropolarimetry of Herbig Ae/Be stars
- Calibrating and Stabilizing Spectropolarimeters with Charge Shuffling and Daytime Sky Measurements
- The Hanle Effect as a Diagnostic of Magnetic Fields in Stellar Envelopes. V. Thin Lines from Keplerian Disks
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