Parameters of very young and massive stars with dust shells |
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| Authors: | Th. Henning |
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| Affiliation: | (1) Universitäts-Sternwarte Jena, G.D.R.;(2) Department of Astronomy and Astrophysics, Charles University, Prague, Czechoslovakia |
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| Abstract: | A radiative transfer model for newly formed hot stars surrounded by optically thick dust shells is applied to a number of compact infrared sources. The model parameters are derived by fitting the synthetic spectra to the observed one between 8 and 13  m and used to derive additional properties of the shells and the embedded stars. |
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