Titlebook: Dust and Molecules in Evolved Stars; Proceedings of an In Isabelle Cherchneff,Tom J. Millar Conference proceedings 1998 Springer Science+Bu

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Was Wilhelm R?pke Really a Proto-Keynesian?etallic grains, the radiation pressure force for a spheroid can be 5–10 times greater than that for a sphere of the same volume..A simple light scattering consideration demonstrates that the distinction in the scattering geometry of aligned non-spherical grains can explain the observed wavelength variations of the positional angle of polarization.

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Theodore Pelagidis,Michael Mitsopoulosnt targets for the study of molecular formation processes. This review presents a compilation of estimated molecular abundances, discusses the uncertainties involved in their estimate, and makes some comparisons with theoretical predictions.

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No Villainous Mother—The Life of Eva Larking disk radii of 10. cm. The dust in such disks is therefore quite cold (near T ~ 50 K for the Red Rectangle) and may emit primarily at submillimeter wavelengths. The disks around stars where there is also substantial . loss may not be easily observable; there could be many as yet undiscovered disks around AGB stars

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Wilhelm R?pke: Why He Was a Conservativeities to allow heavy elements to condense as grains. These dust particles efficiently scatter and absorb stellar photons, transfer the acquired momentum to the ambient gas via collisions and reradiate the absorbed energy at infrared wavelengths.

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