Parameters of very young and massive stars with dust shells

Details Parameters of very young and massive stars with dust shells Parameters of very young and massive stars with dust shells

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.114..401h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 114, no. 2, Sept. 1985, p. 401-411.

Astronomy and Astrophysics

Astrophysics

8

Cosmic Dust, Hot Stars, Radiative Transfer, Stellar Envelopes, Stellar Evolution, Stellar Mass, Stellar Models, Infrared Spectra, Optical Thickness

Scientific paper

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 μm and used to derive
additional properties of the shells and the embedded stars.

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