Dust Shells around OH/IR Stars

We have made new models for mass-losing OH/IR stars to explain the properties of the dust shells around them using more accurate information about the material in the shell and the physical processes including pulsations. We have applied our dust opacity which has been deduced from observations and...

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Bibliographic Details
Main Author: Kyung-Won Suh
Format: Article
Language:English
Published: Korean Space Science Society (KSSS) 1988-12-01
Series:Journal of Astronomy and Space Sciences
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/1988/v5n2/OJOOBS_1988_v5n2_81.pdf