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Continuum Polarization as a Tool: A Perspective for VLT and ALMA

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The Origins of Stars and Planets: The VLT View

Part of the book series: ESO Astrophysics Symposia ((ESO))

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Abstract

We will discuss how polarization maps, obtained with near-infrared imaging instruments such as ISAAC and CONICA/NAOS at the VLT, can be used to determine the structure of star-forming regions.

The analysis of submillimetre polarization maps provided by ALMA will allow the study of magnetic field configurations in the environment of protostars. The potential of submillimetre polarimetry will be demonstrated by a SCUBA polarization map of the globule DC 253-1.6.

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© 2002 Springer-Verlag Berlin Heidelberg

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Henning, T., Launhardt, R., Stecklum, B., Wolf, S. (2002). Continuum Polarization as a Tool: A Perspective for VLT and ALMA. In: Alves, J.F., McCaughrean, M.J. (eds) The Origins of Stars and Planets: The VLT View. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-40277-1_9

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  • DOI: https://doi.org/10.1007/978-3-662-40277-1_9

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-39255-3

  • Online ISBN: 978-3-662-40277-1

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