Amorphous carbon grains and emission spectra of IRC + 10216

Details Amorphous carbon grains and emission spectra of IRC + 10216 Amorphous carbon grains and emission spectra of IRC + 10216

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...231..105o&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 231, no. 1, May 1990, p. 105-110. Research supported by MPI and CNR.

Astronomy and Astrophysics

Astrophysics

22

Amorphous Materials, Emission Spectra, Infrared Radiation, Radiative Transfer, Stellar Envelopes, Carbon, Grain Size, Spectral Bands, Stellar Models

Scientific paper

A simplified model of radiative transfer is applied here to the infrared object IRC + 10216. It is shown that the flux emitted by this source can be explained by considering the presence of amorphous carbon grains around the central star. The stellar parameters of the model are consistent with the variability phases of the central star, and the values of the geometrical and physical parameters of the envelope, deduced from best fits, are in agreement with those obtained elsewhere.

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