Carbon dust particle size distributions around mass-losing AGB stars

Details Carbon dust particle size distributions around mass-losing AGB stars Carbon dust particle size distributions around mass-losing AGB stars

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..402..379j&link_type=abstract

Astrophysical implications of the laboratory study of presolar materials. AIP Conference Proceedings, Volume 402, pp. 379-390 (

Astronomy and Astrophysics

Astrophysics

7

Circumstellar Shells, Clouds, And Expanding Envelopes, Circumstellar Masers, Giant And Subgiant Stars, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, General, Solar Nebula, Cosmogony

Scientific paper

Solids of presolar SiC and interstellar carbon have qualitatively similar relative size distribution for particles with radii, a, in the range 0.35 μm0.35 μm are produced by interacting binary systems rather than single mass-losing stars.

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