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...
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 |
Similar Items
-
Model Dust Envelopes for Asymptotic Giant Branch Stars. I. OH/IR Stars
by: Kyung-Won Suh
Published: (1995-12-01) -
Dust Around T Tauri Stars
by: Kyung-Won Suh, et al.
Published: (2011-12-01) -
Model Dust Envelopes Around Silicate Carbon Stars
by: Kyung-Won Suh
Published: (2006-03-01) -
Aspherical Dust Envelopes Around Oxygen-Rich AGB Stars
by: Kyung-Won Suh
Published: (2006-12-01) -
Models for The IRAS Low Resolution Spectra of OH/IR Stars
by: Sung-Min Lee, et al.
Published: (1998-12-01)