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Linear and Circular Imaging Polarimetry of the Chamaeleon Infrared Nebula

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The Role of Dust in the Formation of Stars

Abstract

We present linear and circular imaging polarimetry observations of the Chamaeleon Infrared Nebula, a bipolar reflection nebula in the Chamaeleon I dark cloud, at near infrared (JHKn) wavelengths. The detection of both high degrees of linear polarisation and a significant degree of circular polarisation in the extended nebulosity allows us to comment on the scattering geometry and the range of particle sizes present.

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© 1996 Springer-Verlag Berlin Heidelberg

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Gledhill, T.M., Chrysostomou, A., Hough, J.H. (1996). Linear and Circular Imaging Polarimetry of the Chamaeleon Infrared Nebula. In: Käufl, H.U., Siebenmorgen, R. (eds) The Role of Dust in the Formation of Stars. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-68594-4_8

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  • DOI: https://doi.org/10.1007/978-3-540-68594-4_8

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-22515-8

  • Online ISBN: 978-3-540-68594-4

  • eBook Packages: Springer Book Archive

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