Siliziumkarbid als möglicher Bestandteil des interstellaren Staubes
作者:
Chr. Friedemann,
期刊:
Astronomische Nachrichten
(WILEY Available online 1968)
卷期:
Volume 291,
issue 4‐5
页码: 177-186
ISSN:0004-6337
年代: 1968
DOI:10.1002/asna.19682910405
出版商: WILEY‐VCH Verlag
数据来源: WILEY
摘要:
AbstractAssuming isothermic atmospheres for the carbon stars, the growth and motion of silicon carbide particles were computed for a set of densities of the atmospheres. It is shown that the particles are able to escape from the atmosphere in case the surface acceleration is sufficiently low. An estimation of the whole mass of the expelled particles points out that only a small fraction of the interstellar dust can be silicon carbide. Nevertheless it is possible that these particles could act as condensation cores in the interstellar space.
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