Interstellar Dust Models Consistent with Extinction, Infrared Emission, Abundances, Albedo, and X-ray Scattering Constraints

Details Interstellar Dust Models Consistent with Extinction, Infrared Emission, Abundances, Albedo, and X-ray Scattering Constraints Interstellar Dust Models Consistent with Extinction, Infrared Emission, Abundances, Albedo, and X-ray Scattering Constraints

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21560629f&link_type=abstract

American Astronomical Society, AAS Meeting #215, #606.29; Bulletin of the American Astronomical Society, Vol. 36, p.1134

Astronomy and Astrophysics

Astronomy

Scientific paper

We use classical inversion techniques to derive the size distributions
and abundances of interstellar dust consisting of graphite and silicate
grains and polycyclic aromatic hydrocarbons (PAHs), using the average
interstellar extinction, infrared emission, and abundances, as well as
their albedo, and X-ray scattering observations as constraints.

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