Abstract
In this paper, the properties of circumstellar dust grains located in the environment of young stellar objects will be reviewed. After a short introduction to the field of young stellar objects, the main results of infrared spectroscopy will be discussed. Infrared and millimetre continuum observations form a further topic of this paper. The properties of recent dust models for cocoons and accretion disks are summarized with special emphasis on the dust opacities at millimetre wavelengths.
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Henning, T. (1996). Dust Around Young Stellar Objects. In: Greenberg, J.M. (eds) The Cosmic Dust Connection. NATO ASI Series, vol 487. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5652-3_30
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DOI: https://doi.org/10.1007/978-94-011-5652-3_30
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