HL Tau: 3-D Polarisation Modelling and Magnetic Field Structure

Lucas, P.W., Fukagawa, M., Tamura, M., Chrysostomou, A. and Beckford, A. (2005) HL Tau: 3-D Polarisation Modelling and Magnetic Field Structure. In: UNSPECIFIED.

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We describe 3-dimensional Monte Carlo modelling of HL Tau in the near infrared with aligned non-spherical grains. JHK linear polarimetry with 0.4-0.6 arcsec resolution from Subaru and UKIRT is fitted in detail, providing information about the structure of the system, the grain properties and perhaps also the magnetic field. Circular polarisation models are also presented, showing how near infrared circular polarimetry will provide the key to measuring magnetic field structure in protostars on the scale of the solar system, provided that circular polarimeters become available. This is illustrated with recently obtained circular polarimetry of the intermediate mass YSO HH135.

Item Type	Conference or Workshop Item (Other)
Additional information	Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html Copyright ASP
Date Deposited	15 May 2025 16:19
Last Modified	04 Feb 2026 00:15