Physical Properties of Submicronic Carbonaceous Particles Candidate as Cosmic Dust-Reference-Cited by-同舟云学术

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Physical Properties of Submicronic Carbonaceous Particles Candidate as Cosmic Dust

Published:1985 Issue: Volume:85 Page:159-162
ISSN:0252-9211
Container-title:International Astronomical Union Colloquium
language:en
Short-container-title:International Astronomical Union Colloquium

Author:

Borghesi A.,Bussoletti E.,Colangeli L.

Abstract

AbstractWe present here a compendium of our laboratory measurements of the physical properties of submicronic particles made by some carbonaceous materials candidate as cosmic dust: amorphous carbon, silicon carbide. Comparison with data obtained by other authors is presented and discussed in view of astrophysical applications.

Publisher

Cambridge University Press (CUP)

Reference13 articles.

1. Origin of Amorphous Interstellar Grains

2. Visible and ultraviolet /800-130 nm/ extinction of vapor-condensed silicate, carbon, and silicon carbide smokes and the interstellar extinction curve

3. The 2200 � extinction hump and porous graphite grains

4. Effects of physical adsorption on porous interstellar grains

5. The absorption efficiency of submicron amorphous carbon particles between 2.5 and 40 μm

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Introduction;Synthetic Impulse and Aperture Radar (SIAR);2014-01-17

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