Re-calculation of the Pollack et al. (1994), ApJ 421, 615-639
results
- using their optical constants and
- assuming a modified MRN dust size distribution
- for chemically homogeneous compact
spheres,
- for chemically homogeneous dust
aggregates,
- for chemically inhomogeneous dust
aggregates.
Back to the general home page of
Astronomy and Astrophysics in Jena.
Created by
R. Stognienko,
Dec 1996