Spectroscopic Study of Carbon Stars with the ISO-SWS

被引：0
|
作者：
K. Justtanont
J. Cami
I. Yamamura
T. De Jong
L.B.F.M. Waters
机构：
[1] SRON,Department of Astronomy
[2] University of Tokyo,Astronomical Institute
[3] University of Amsterdam,undefined
来源：
Astrophysics and Space Science | 1997年 / 255卷 / 1-2期
关键词：
Color; Dust; Infrared Spectrum; Energy Distribution; Short Wavelength;
D O I：
10.1023/A:1001504311386
中图分类号：
学科分类号：
摘要：
We have observed ten carbon stars with different mass-loss rates using the Short Wavelength Spectrometer (SWS) on board ISO. We found that not only the spectral energy distribution and the dust features, but that also that the strength and/or shape of molecular absorption features in the infrared spectrum varies with the near-infrared color temperature, i.e. with the thickness of the circumstellar envelope.
引用
收藏
页码：351 / 357
页数：6
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