Monte-Carlo simulations of linear polarization in clumpy OB-star winds

Type Conference Paper
Names Richard H. D. Townsend, Nick Mast
Conference Name IAU Symposium
Volume 272
Pages 216-217
Date July 1, 2011
Library Catalog NASA ADS
Abstract We present results from Monte-Carlo simulations of linear polarization in clumped OB-star winds. We find that previous single-scattering models of clumped winds have overestimated the degree of polarization, even in cases where individual clumps are optically thin. An application to P Cygni suggests the star's wind is more fragmented than previously thought.
Tags Methods: Numerical, Polarization, RADIATIVE TRANSFER, SCATTERING, Stars: Mass Loss, Techniques: Polarimetric, outflows, stars: early-type, stars: individual (P Cygni), stars: winds
UW-Madison Astronomy Home