Astronomy and Astrophysics – Astronomy
Scientific paper
May 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994dib..nasa...11f&link_type=abstract
In NASA. Ames Research Center, The Diffuse Interstellar Bands: Contributed Papers p 11-16 (SEE N95-15827 03-89)
Astronomy and Astrophysics
Astronomy
Absorption Spectra, Astronomy, Diffuse Radiation, Interplanetary Dust, Magellanic Clouds, Monte Carlo Method, Radiation Transport, Reflection Nebulae, Stellar Spectra, Astronomical Models, Interstellar Extinction, Light Scattering, Light Transmission, Refractivity, Wavelengths
Scientific paper
A Monte Carlo code for radiation transport calculations is used to compare the profiles of the lambda lambda 5780 and 6613 Angstrom diffuse interstellar bands in the transmitted and the reflected light of a star embedded within an optically thin dust cloud. In addition, the behavior of polarization across the bands were calculated. The wavelength dependent complex indices of refraction across the bands were derived from the embedded cavity model. In view of the existence of different families of diffuse interstellar bands the question of other parameters of influence is addressed in short.
Fischer Oystein
Henning Thomas
Pfau Werner
Stognienko R.
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